cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Melanotis caerulescens subsp. longirostris
Creators: name: Silva, Héctor Gómez de
name: Pérez Villafaña, Mónica G.
name: Cruz-Nieto, Javier
name: Cruz-Nieto, Miguel Ángel
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Mimidae
Melanotis
Melanotis caerulescens
Melanotis caerulescens longirostris

description: BLUE MOCKINGBIRD Melanotis caerulescens longirostris
 (vs. M. c. caerulescens total score 4)
 Coloration.—Based on 52 male and 24 female longirostris vs. 29 male and 32 female caerulescens, Grant (1965a) found that ‘less than half’ of longirostris were paler in the throat and crown feathers than ‘most’ of his caerulescens sample but the palest specimens of each were indistinguishable. Therefore there is large overlap (no score).
 Morphometrics.—Slightly larger but has proportionately much longer bill in both sexes (score 2) whereas the tail is shorter, especially in males (score 2). Additionally, Grant (1965a) found that coracoid length may be shorter in island birds but did not provide sufficient information to calculate effect size because he considered his sample to be inadequate (three male and six female longirostris vs. five male and two female caerulescens). However, the measurement ranges have slight to no overlap, which suggest the difference is not minor (not scored).
description: Published as part of Silva, Héctor Gómez de, Pérez Villafaña, Mónica G., Cruz-Nieto, Javier & Cruz-Nieto, Miguel Ángel, 2020, Are some of the birds endemic to the Tres Marías Islands (Mexico) species?, pp. 7-37 in Bulletin of the British Ornithologists' Club 140 (1) on page 25, DOI: 10.25226/bboc.v140i1.2020.a3, http://zenodo.org/record/13755707
NEAR – technical analysis and lessons learned from a unique experiment
Creators: name: Kasper, Markus
Publisher: name: Zenodo
Year: 2020

description: In June 2019, ESO and the Breakthrough Initiatives carried out the NEAR experiment, a 100-hour campaign to search for low-mass planets in the Alpha Centauri system, utilizing high-contrast imaging in the thermal IR. This has been made possible by moving VISIR to the VLT-UT4 and using the Deformable Secondary Mirror for AO and N-band AGPM coronagraphy. We will present the NEAR concept, and report on the achieved sensitivity and contrast. The expected performance of NEAR will allow us to probe down to the mini-Neptune range, while reaching down to a true Earth analogue would require a more sensitive detector technology and multiple telescopes observing in concert. We will report on the data reduction efforts carried out by several independent teams, and present campaign results.
Baseline report on present skills gaps in shipbuilding and offshore renewables value chains
Creators: name: Sdoukopoulos, Eleftherios
name: Tsafonias, Giorgos
name: Perra, Vasiliki-Maria
name: Boile, Maria
Publisher: name: Zenodo
Year: 2020
Subjects: skill gaps
offshore renewable energy
shipbuilding
maritime technologies
skills mismatch
skills strategy

description: The objective of the MATES Baseline Report on Present Skill Gaps is to deliver a critical review and analysis of the skills supply and demand mismatch in Europe for the two sectors addressed i.e. shipbuilding and offshore renewable energy. The report is the result of extensive desktop research, industry engagement through regional workshops, a validation workshop, surveys, expert interviews, Focus Group meetings and builds upon the MATES State of the Art Report (D1.2).
On the history of ground-based thermal-IR astronomy
Creators: name: Käufl, Hans-Ulrich
Publisher: name: Zenodo
Year: 2020

description: Since ~1980 until today, almost without interruption, ESO has been offering, state of the art thermal IR facility class instrumentation to its community. There was a stunning evolution from single pixel detectors to EFOSC/FORS-like multi mode instrumentation including high resolution Echelle spectroscopy. This was possible due to a rapid technical evolution in the fields of cryogenics and detectors. This allowed the adoption of classical optical designs, such as EFOSC to be used in a field then, and today(?), considered at best "exotic" by most astronomers. The ESO LaSilla instrumentation was the perfect match to Europe's groundbreaking infrared missions, the IRAS satellite and the ISO, the infrared space observatory.
Letter from Michael J. Grizer to Mark Wolfe, Rehabilitation of Building 134, Fort Sam Houston, Texas
Creators: name: Grizer, Michael J.
Publisher: name: Department of the Air Force
Year: 2011
Subjects: subject: JBSA-Sam Houston
valueUri: https://core.tdar.org/browse/geographic-keyword/82532/jbsa-sam-houston
subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Bexar (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/4150/bexar-county
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Fort Sam Houston National Historic Landmark District
valueUri: https://core.tdar.org/browse/geographic-keyword/82955/fort-sam-houston-national-historic-landmark-district
subject: Historic
valueUri: https://core.tdar.org/browse/culture-keyword/25/historic
subject: Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/318/governmental-structure
subject: Historic Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/320/historic-governmental-structure
subject: Military Structure
valueUri: https://core.tdar.org/browse/site-type/322/military-structure
subject: NRHP
valueUri: https://core.tdar.org/browse/other-keyword/9857/nrhp
subject: Administration
valueUri: https://core.tdar.org/browse/other-keyword/56323/administration
subject: Troop Barracks
valueUri: https://core.tdar.org/browse/other-keyword/156854/troop-barracks
subject: Building 134
valueUri: https://core.tdar.org/browse/other-keyword/146284/building-134
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: Joint Base San Antonio, Fort Sam Houston, is proposing an undertaking to rehabilitate building 134. Constructed in 1905 as troop barracks, the building has long been used as administrative space. Building 134 is a property eligible for the National Register of Historic Places and is within Fort Sam Houston’s National Historic Landmark District. After careful examination of this proposal, the JB-SA Cultural Resource Staff has determined this undertaking will result in no adverse effect and the rehabilitation of this facility will assure its long term use and utility.
Structural phase transitions in the kagome lattice based materials Cs2-xRbxSnCu3F12 (x = 0, 0.5, 1.0, 1.5)
Creators: name: Downie, L. J.
name: Black, C.
name: Ardashnikova, E. I.
name: Tang, C. C.
name: Vasiliev, A. N.
name: Golovanov, A. N.
name: Berdonosov, P. S.
name: Dolgikh, V. A.
name: Lightfoot, P.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: The solid solution Cs2-xRbxSnCu3F12 (x = 0, 0.5, 1.0, 1.5) has been investigated crystallographically between 100 and 300 K using synchrotron X-ray powder diffraction and, in the case of x = 0, neutron powder diffraction.
description: 14 pages, 9 figures
VLT/VISIR Calibration programme and stray light modeling
Creators: name: Politopoulos, Ioannis
name: Burtscher, Leonard
Publisher: name: Zenodo
Year: 2020

description: Talk with accompanying poster. For decades, the standard background subtraction scheme in ground-based thermal-infrared observations has been a combination of chopping and nodding. Since the thermal background stability of the ELT during nodding is currently unclear, we investigate an alternative background subtraction scheme using only chopping. Using data from VLT/VISIR we study the structure in chop-difference frames which is dominated by a gradient. In this research we determine the origin of this gradient with the aim to understand, qualitatively and quantitatively, the link between telescope structure and chopping residuals. To achieve that, we construct a simple model which describes the most significant warm emitter in the VLT pupil seen by VISIR (the folded M3 tower) and show that this structure is responsible for the observed gradient in the chopping residuals. We corroborate our findings by implementing this model -- and reproducing the effect -- in the ray-tracing software FRED.
(:unas) unassigned
Creators: name: (:Unkn) Unknown
Publisher: name: Universita' degli Studi di Salerno
Year: 2024

description: The present paper examines one of the most famous female figures of the Kabyle/ Amazigh mythology, Lunja who has been invisible in the mainstream of academic concerns in Algeria and abroad. The few studies carried on the topic often portrayed her as a voiceless, submissive and an obedient beautiful young girl. We shall, however, try to “deconstruct” the prevailing fabricated image of this mythological character, Lunja, by emphasizing her various strategies of resistance and deviation of oppression. We shall also move beyond the previous approaches to history that narrates the relationship between Lunja and Teryel, her mother based solely on a dichotomy that has been described by the few studies since the old times. The objective is to show that Lunja’s performativityof silence is a technique with which she bypasses the constraints of her traditional society in transgressing its well established norms through actions. In so doing, Lunja can be regarded then as a female trickster and a subversive figure, who constantly calls into question the established order for the sake of changing her status quo. The analysis is mainly based on ideas and concepts such as gender performativity, which are provided in Judith Butler’s book entitled, Gender Trouble (1990). We also appropriate features and the image of Trickster according to Robert Pelton to show how the Kabyle/ Amazigh mythological figure Lunja constantly re-values the traditional norms and values through subversive actions that make her join the family of the female tricksters.
Sonnenfleckenzeichnung Nr. 94.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 25.04.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Time-correlation between the radio and gamma-ray activity in blazars and the production site of the gamma-ray emission
Creators: name: Max-Moerbeck, W.
name: Hovatta, T.
name: Richards, J. L.
name: King, O. G.
name: Pearson, T. J.
name: Readhead, A. C. S.
name: Reeves, R.
name: Shepherd, M. C.
name: Stevenson, M. A.
name: Angelakis, E.
name: Fuhrmann, L.
name: Grainge, K. J. B.
name: Pavlidou, V.
name: Romani, R. W.
name: Zensus, J. A.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: In order to determine the location of the gamma-ray emission site in blazars, we investigate the time-domain relationship between their radio and gamma-ray emission. Light-curves for the brightest detected blazars from the first 3 years of the mission of the Fermi Gamma-ray Space Telescope are cross-correlated with 4 years of 15GHz observations from the OVRO 40-m monitoring program. The large sample and long light-curve duration enable us to carry out a statistically robust analysis of the significance of the cross-correlations, which is investigated using Monte Carlo simulations including the uneven sampling and noise properties of the light-curves. Modeling the light-curves as red noise processes with power-law power spectral densities, we find that only one of 41 sources with high quality data in both bands shows correlations with significance larger than 3-sigma (AO 0235+164), with only two more larger than even 2.25-sigma (PKS 1502+106 and B2 2308+34). Additionally, we find correlated variability in Mrk 421 when including a strong flare that occurred in July-September 2012. These results demonstrate very clearly the difficulty of measuring statistically robust multiwavelength correlations and the care needed when comparing light-curves even when many years of data are used. This should be a caution. In all four sources the radio variations lag the gamma-ray variations, suggesting that the gamma-ray emission originates upstream of the radio emission. Continuous simultaneous monitoring over a longer time period is required to obtain high significance levels in cross-correlations between gamma-ray and radio variability in most blazars.
description: 8 pages, 3 figures and 2 tables. Accepted for publication in MNRAS
Memorandum of Agreement between Randolph Air Force Base and The Texas Historical Commission and the Advisory Council on Historic Preservation
Creators: name: Peterson, Donald L.
Publisher: name: Randolph Air Force Base
Year: 1993
Subjects: subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Randolph Air Force Base
valueUri: https://core.tdar.org/browse/geographic-keyword/78971/randolph-air-force-base
subject: Building 901
valueUri: https://core.tdar.org/browse/other-keyword/146466/building-901
subject: Building 907
valueUri: https://core.tdar.org/browse/other-keyword/146471/building-907
subject: Building 903
valueUri: https://core.tdar.org/browse/other-keyword/153691/building-903
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: Randolph Air Force Base has determined that a project to rehabilitate Buildings 901, 903, and 907 will have an effect upon these properties eligible for inclusion in the National Register of Historic Places, and has consulted with the State of Texas, State Historic Preservation Officer and the Advisory Council on Historic Preservation. The mentioned parties agree that the project shall be implemented in accordance with the following stipulations in order to take into account the effect of the undertaking on historic properties.
D4.12 Interim report on the information architecture of the Copyright User EU site
Creators: name: Meletti, Bartolomeo
Publisher: name: Zenodo
Year: 2021
Subjects: copyright
EU
user

description: Task 4.4 – Copyright User: Designing the EU Copyright Guidance Portal is part of Work Package 4 – Creative Industries. This interim report on the information architecture of the CopyrightUser.eu site is the main output of subtask 4.4.1 (D4.12 – Interim report on the information architecture of the Copyright User EU site). Section 1 – Introduction and methodology introduces the Copyright User initiative and describes its methodological approach. After shortly reporting the evolution of the information architecture of the CopyrightUser.org website, Section 2 – Information architecture outlines the basic structure and potential developments of CopyrightUser.eu. Finally, Section 3 – Conclusions summarises the next steps of Task 4.4. Please note: a screen-reader accessible version of this report can be downloaded via this link https://docs.google.com/uc?export=download&id=1xQeQagiaXiJg5VkprwMoMQf1hhG464cl
Sonnenfleckenzeichnung Nr. 27.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 10.02.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
title: Wie schätzen Lehrkräfte die Lernstandserhebungen in Mathematik ein?
title: Projektevaluation, Typisierung und Ist-Stand zu Einstellungen zu den Lernstandserhebungen Mathematik Klasse 8 in Hessen
Creators: name: Vogel, Sebastian
Publisher: name: Universität Kassel
Year: 2020
Subjects: subject: Lehrerfortbildung
subject: Lernstandserhebungen
subject: VerA
subject: Vergleichsarbeiten
subject: Evaluation
subject: Typisierung
subject: 370
subject: Lehrerfortbildung
subject: Schulleistungsmessung
subject: Mathematikunterricht
subject: Schuljahr 8
subject: VERA
subject: Evaluation
subject: Typisierung

description: Zugleich: Dissertation, Universität Kassel, 2018
Sonnenfleckenzeichnung Nr. 201.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 23.08.1988, 07:15, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
OAHP Inventory, Building 4168 Maintenance Shop, Fort Sam Houston, Texas
Creators: name: Walter, Chelsea
Publisher: name: Office of Archaeology and Historic Preservation
Year: 1978
Subjects: subject: Fort Sam Houston
valueUri: https://core.tdar.org/browse/geographic-keyword/83681/fort-sam-houston
subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Bexar (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/4150/bexar-county
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Historic
valueUri: https://core.tdar.org/browse/culture-keyword/25/historic
subject: Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/318/governmental-structure
subject: Historic Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/320/historic-governmental-structure
subject: Non-Domestic Structures
valueUri: https://core.tdar.org/browse/site-type/309/non-domestic-structures
subject: OAHP
valueUri: https://core.tdar.org/browse/other-keyword/138292/oahp
subject: Building 4168
valueUri: https://core.tdar.org/browse/other-keyword/146652/building-4168
subject: Maintenance Shop
valueUri: https://core.tdar.org/browse/other-keyword/159132/maintenance-shop
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: An inventory form by the Office of Archaeology and Historic Preservation for Building 4168 at Fort Sam Houston, Texas. The structure was built in 1934 as a maintenance shop.
Sonnenfleckenzeichnung Nr. 65.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 20.03.1988, 10:15, erstellt von Marco Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Husimi distribution and phase space analysis of Dicke model quantum phase transition
Creators: name: Romera, E.
name: del Real, R.
name: Calixto, M.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The Husimi distribution is proposed for a phase space analysis of quantum phase transitions in the Dicke model of spin-boson interactions. We show that the inverse participation ratio and Wehrl entropy of the Husimi distribution give sharp signatures of the quantum phase transition. The analysis has been done using two frameworks: a numerical treatment and an analytical variational approximation. Additionally we have proposed a new characterization of the Dicke model quantum phase transition by means of the zeros of the Husimi distribution in the variational approach.
description: arXiv admin note: substantial text overlap with arXiv:1409.5789, arXiv:1409.5591
Sonnenfleckenzeichnung Nr. 174.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 26.07.1988, 06:45, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
CEV Project Coordination Form, Exterior Renovation Building 118, Randolph Air Force Base, Texas
Creators: name: Walter, Chelsea
Year: 1998
Subjects: subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Bexar (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/4150/bexar-county
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Randolph Air Force Base
valueUri: https://core.tdar.org/browse/geographic-keyword/78971/randolph-air-force-base
subject: Historic
valueUri: https://core.tdar.org/browse/culture-keyword/25/historic
subject: Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/318/governmental-structure
subject: Historic Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/320/historic-governmental-structure
subject: Building 118
valueUri: https://core.tdar.org/browse/other-keyword/146269/building-118
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: The office of the SHPO was given the opportunity to comment on the project to renovate the exterior of Building 118. Modification to the building’s facade as shown in the attached elevation was deleted. The revised elevation was sent to the office of the SHPO. If these conditions are met Section 106 coordination is complete.
SEP acceleration in CME driven shocks using a hybrid code
Creators: name: Gargate, L.
name: Fonseca, R. A.
name: Silva, L. O.
name: Bamford, R. A.
name: Bingham, R.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We preform hybrid simulations of super Alfvenic quasi-parallel shock, driven by a Coronal Mass Ejection (CME), propagating in the Outer Coronal or Solar Wind at distances of between 3 to 6 solar radii. The hybrid treatment of the problem enable the study of the shock propagation on the ion time scale, preserving ion kinetics and allowing for a self consistent treatment of the shock propagation and particle acceleration. The CME plasma drags the embedded magnetic field lines stretching from the sun, and propagates out into interplanetary space at a greater velocity than the in-situ solar wind, driving the shock, and producing very energetic particles. Our results show electromagnetic Alfven waves are generated at the shock front. The waves propagate upstream of the shock and are produced by the counter streaming ions of the solar wind plasma being reflected at the shock. A significant fraction of the particles are accelerated in two distinct phases: first, particles drift from the shock and are accelerated in the upstream region and, second, particles arriving at the shock get trapped, and are accelerated at the shock front. A fraction of the particles diffused back to the shock, which is consistent with the Fermi acceleration mechanism.
description: Accepted for publication in Astrophysical Journal 18th June 2014
Sonnenfleckenzeichnung Nr. 313.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 31.12.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 36.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.02.1988, 08:15, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 41.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 24.02.1988, 08:30, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 107.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.05.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 4.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Sonnenfleckenzeichnung Nr. 125.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 02.06.1988, 07:00, erstellt von Marco Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
A method for the estimation of the significance of cross-correlations in unevenly sampled red-noise time series
Creators: name: Max-Moerbeck, W.
name: Richards, J. L.
name: Hovatta, T.
name: Pavlidou, V.
name: Pearson, T. J.
name: Readhead, A. C. S.
Publisher: name: arXiv
Year: 2014
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: We present a practical implementation of a Monte Carlo method to estimate the significance of cross-correlations in unevenly sampled time series of data, whose statistical properties are modeled with a simple power-law power spectral density. This implementation builds on published methods, we introduce a number of improvements in the normalization of the cross-correlation function estimate and a bootstrap method for estimating the significance of the cross-correlations. A closely related matter is the estimation of a model for the light curves, which is critical for the significance estimates. We present a graphical and quantitative demonstration that uses simulations to show how common it is to get high cross-correlations for unrelated light curves with steep power spectral densities. This demonstration highlights the dangers of interpreting them as signs of a physical connection. We show that by using interpolation and the Hanning sampling window function we are able to reduce the effects of red-noise leakage and to recover steep simple power-law power spectral densities. We also introduce the use of a Neyman construction for the estimation of the errors in the power-law index of the power spectral density. This method provides a consistent way to estimate the significance of cross-correlations in unevenly sampled time series of data.
description: 24 pages, 30 figures and 2 tables. Accepted for publication in MNRAS
Sonnenfleckenzeichnung Nr. 298.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 15.12.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
(:unas) unassigned
Creators: name: (:Unkn) Unknown
Publisher: name: Universita' degli Studi di Salerno
Year: 2024

description: La fantasia è una facoltà mentale a cui la monaca di Monza, prima della professione religiosa, ricorre con frequenza. Nel Fermo e Lucia, anche a causa della sua scarsa abilità di instaurare relazioni con gli altri personaggi, Geltrude è spesso succube delle proprie fantasie, che si impongono nella mente e la distolgono dagli eventi reali. La giovane, tuttavia, non tenta di liberarsene, poiché grazie ad esse può immaginare una vita in cui coltivare al massimo grado l’orgoglio nobiliare, secondo l’educazione ricevuta in famiglia. Nella prima parte di questo articolo sono commentate, inoltre, alcune varianti significative del manoscritto di prima minuta che, anche solo con la sostituzione di un singolo termine o di brevi sintagmi, arricchiscono di maggiori dettagli la narrazione. Nei Promessi Sposi, l’avvenire da monaca della giovane è imposto con più forza dal padre rispetto al Fermo. Gertrude, consapevole di non poter decidere il proprio futuro, ricorre alla fantasia per immaginare, peraltro in maniera infruttuosa, una vita nel secolo, secondo i propri desideri.
description: The monaca di Monza, before her religious profession, makes oftentimes use of fancy as a mental faculty. In Fermo e Lucia, also because of her poor relational ability with the other characters, Geltrude is frequently victim of her fancies, which are able to lead her thoughts and take her away from reality. Nevertheless, the girl does not even try to get herself rid of it, as thank to these mental images she can dream a life in which she could cherish to the maximum extent her pride to be an aristocratic, according to the kind of education she received by her family. In the first part of this essay, are furthermore commented some relevant variant readings found in the first draft manuscript which add more details to the story, even with the substitution of only one word or of brief phrases. In I Promessi Sposi, the monastic future of the girl is more strictly forced by the father compared to what happens in Fermo e Lucia. Gertrude, knowing that she is not able to choose her life freely, makes use of fancy to imagine, though without success, a life according to her desires, in the outside world.
Rural Conditions and Trends
Creators: name: USDA ERS
name: USDA ERS
Publisher: name: Unknown
Year: 1991
Subjects: Community/Rural/Urban Development

description: Overview: Recession Hits Rural Areas No Harder than Urban; National Economic Conditions: Recovery Gains Ground; Employment: Rural Employment Down; Unemployment: Rural Employment Up in First Half of 1991; Appendix: Data Sources and Definitions; Appendix Tables
Sonnenfleckenzeichnung Nr. 297.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 14.12.1988, 09:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
Cardinalis cardinalis subsp. mariae Nelson 1898
Creators: name: Silva, Héctor Gómez de
name: Pérez Villafaña, Mónica G.
name: Cruz-Nieto, Javier
name: Cruz-Nieto, Miguel Ángel
Publisher: name: Zenodo
Year: 2020
Subjects: Biodiversity
Taxonomy
Animalia
Chordata
Aves
Passeriformes
Cardinalidae
Cardinalis
Cardinalis cardinalis
Cardinalis cardinalis mariae

description: NORTHERN CARDINAL Cardinalis cardinalis mariae
 (vs. C. c. affinis)
 Coloration.—Based on 44 male and 35 female mariae vs. ten male and six female affinis, Grant (1965a) reported that 92% of males had a purple tinge to the plumage vs. 100% without any purple tinge (score 1), 100% of mariae females had cream-white abdomens vs. pale buff in 83% (score 1); and the grey chin and throat of females covered a larger area vs. more restricted white or rarely grey chin (score 2, grey is caused by ‘the black basal half of the feather showing through the overlying white feather-tips, and in island specimens the extent of white in the feather tip is reduced’).
 Morphometrics.—Longer wing, tarsus and bill (especially bill length in males) (score 2) but shorter tail (score 2). Bill more bulging (consistent with Ridgway 1901 [not scored]).
 Additional information.— Smith et al. (2011), Smith & Klicka (2013) and Ortiz-Ramírez et al. (2018) found reciprocal monophyly and deep genetic divergence between mariae and mainland specimens. Smith & Klicka (2013) and Ortiz-Ramírez et al. (2018) reported that small population size has accelerated molecular evolution in mariae.
 Reasons for uncertainty.— Grant’s (1965a) sample of affinis was inadequate (morphometric characters were evaluated in 4– 9 males and six females, and plumage characters in ten males and six females), which is especially problematic because female plumage apparently fades considerably in specimens and males display extensive individual variation (Van Rossem 1932). Furthermore, Baja California race igneus is as likely to be the sister species of mariae as affinis, and it was not explicitly compared by Grant (1965a) who stated only that ‘ five specimens of igneus were available too, and it was noted that [mariae] differed from both subspecies (igneus and affinis) mainly in the same way.’ Nelson (1898) in the original description of mariae described it as being closest to igneus, and at least in bill shape it is intermediate between mariae and affinis (Ridgway 1901: 648–649). Ortiz-Ramírez et al. (2018: 726) mentioned that when analysing the haplotype network, mariae was closer to igneus than affinis, although this apparently contradicts both their own highest-probability scenario of colonisation (in their Fig. 4) and the phylogenies of Smith et al. (2011) and Smith & Klicka (2013). Therefore, this case requires further study.
description: Published as part of Silva, Héctor Gómez de, Pérez Villafaña, Mónica G., Cruz-Nieto, Javier & Cruz-Nieto, Miguel Ángel, 2020, Are some of the birds endemic to the Tres Marías Islands (Mexico) species?, pp. 7-37 in Bulletin of the British Ornithologists' Club 140 (1) on page 33, DOI: 10.25226/bboc.v140i1.2020.a3, http://zenodo.org/record/13755707
Finite temperature quark-gluon vertex with a magnetic field in the Hard Thermal Loop approximation
Creators: name: Ayala, Alejandro
name: Cobos-Martinez, J. J.
name: Loewe, M.
name: Tejeda-Yeomans, Maria Elena
name: Zamora, R.
Publisher: name: arXiv
Year: 2014
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: High Energy Physics - Lattice (hep-lat)
subject: High Energy Physics - Theory (hep-th)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: We compute the thermo-magnetic correction to the quark-gluon vertex in the presence of a weak magnetic field within the Hard Thermal Loop approximation. The vertex satisfies a QED-like Ward identity with the quark self-energy. The only vertex components that get modified are the longitudinal ones. The calculation provides a first principles result for the quark anomalous magnetic moment at high temperature in a weak magnetic field. We extract the effective thermo-magnetic quark-gluon coupling and show that this decreases as a function of the field strength. The result supports the idea that the properties of the effective quark-gluon coupling in the presence of a magnetic field are an important ingredient to understand the inverse magnetic catalysis phenomenon.
description: 9 pages, 4 figures
Sonnenfleckenzeichnung Nr. 13.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 19.01.1988, 14:45, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 3.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)
OAHP Inventory, Building 601 and Building 602 Infantry Post and Company Barracks, Fort Sam Houston, Texas
Creators: name: Walter, Chelsea
Publisher: name: Office of Archaeology and Historic Preservation
Year: 1978
Subjects: subject: Fort Sam Houston
valueUri: https://core.tdar.org/browse/geographic-keyword/83681/fort-sam-houston
subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Bexar (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/4150/bexar-county
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Historic
valueUri: https://core.tdar.org/browse/culture-keyword/25/historic
subject: Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/318/governmental-structure
subject: Historic Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/320/historic-governmental-structure
subject: Non-Domestic Structures
valueUri: https://core.tdar.org/browse/site-type/309/non-domestic-structures
subject: OAHP
valueUri: https://core.tdar.org/browse/other-keyword/138292/oahp
subject: Building 601
valueUri: https://core.tdar.org/browse/other-keyword/146372/building-601
subject: Company Barrack
valueUri: https://core.tdar.org/browse/other-keyword/152866/company-barrack
subject: Building 602
valueUri: https://core.tdar.org/browse/other-keyword/146373/building-602
subject: Infantry Post
valueUri: https://core.tdar.org/browse/other-keyword/154363/infantry-post
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Architectural Survey
valueUri: https://core.tdar.org/browse/investigation-type/2/architectural-survey
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: An inventory form by the Office of Archaeology and Historic Preservation for Building 601 and Building 602 at Fort Sam Houston, Texas. The structures were built in 1890 as an infantry post and company barracks.
Correspondence Packet, Rehabilitation of First Floor and Basement of Building 671, Randolph Air Force Base, Texas
Creators: name: Walter, Chelsea
Year: 1992
Subjects: subject: San Antonio
valueUri: https://core.tdar.org/browse/geographic-keyword/4149/san-antonio
subject: Bexar (County)
valueUri: https://core.tdar.org/browse/geographic-keyword/4150/bexar-county
subject: Texas
valueUri: https://core.tdar.org/browse/geographic-keyword/6923/texas
subject: Randolph Air Force Base
valueUri: https://core.tdar.org/browse/geographic-keyword/78971/randolph-air-force-base
subject: Historic
valueUri: https://core.tdar.org/browse/culture-keyword/25/historic
subject: Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/318/governmental-structure
subject: Historic Governmental Structure
valueUri: https://core.tdar.org/browse/site-type/320/historic-governmental-structure
subject: Non-Domestic Structures
valueUri: https://core.tdar.org/browse/site-type/309/non-domestic-structures
subject: Building 671
valueUri: https://core.tdar.org/browse/other-keyword/146452/building-671
subject: Architectural Documentation
valueUri: https://core.tdar.org/browse/investigation-type/16/architectural-documentation
subject: Heritage Management
valueUri: https://core.tdar.org/browse/investigation-type/24/heritage-management

description: A group of letters and supporting documentation for the proposed undertaking to rehabilitate the interior of the first floor and basement at Building 671, Randolph Air Force Base, Texas. Summary documentation in the attachments include location maps, historic data, photographs, drawings, and the undertaking description and assessment.
Sonnenfleckenzeichnung Nr. 241.
Zeichnung von Flecken und Fackelflächen zur Ermittlung der Sonnenaktivität am 07.10.1988, 15:00, erstellt von Sergio Cortesi, Sonnenobservatorium Specola Solare Ticinese in Locarno
Creators: name: Observatorium Specola Solare Ticinese Locarno (1957 bis 1980 Teil der Eidgenössischen Sternwarte der ETH Zürich)
Publisher: name: [s.n.]
Year: 1988

description: Bleistiftzeichnung mit schwarzer Farbe und Bleistift, erstellt als Projektionsbildzeichnung für die Beobachtungen in Locarno-Monti auf einem eigenen Vordruck. Instrument: Zeiss-Coudé-Refraktor mit 15 cm Öffnung und 225 cm Brennweite. Bildqualität (SIDC): 2.
Die Beobachtungen zu Einzelflecken und zu Sonnenfleckengruppen wurden auf dem Vordruck eingetragen. Zusätzlich sind zuhanden der späteren statistischen Verarbeitung die Angaben für die Bestimmung der Fleckenrelativzahl notiert.
Beobachtungstätigkeit unter eigenständiger Leitung (Associazione Specola Solare Ticinese ASST)