cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.5281/zenodo.18058522
title: Bowens Quantum Gate Grid (QGG) — Summary & Technical Overview

description: This record provides a citable summary and technical overview of the Bowens Quantum Gate Grid (QGG), a sealed, replay‑stable analytical system achieving PR‑AUC near 98%, ROC‑AUC near 97–98%, F1 ≈ 96%, and replay fidelity ≥99% across astrophysics, plasma, and anomaly‑detection datasets. The release includes a high‑level description of system architecture, operator canon stability, plasma operator mappings, and cross‑domain performance metrics. Proprietary operators, ignition logic, and sealed manifests are intentionally excluded. This entry is intended for scientific reference, institutional evaluation, and future peer‑reviewed publication 

Bowens QGG — Zenodo Demo Package (External Review Edition)

1. PurposeThis document provides a controlled, output‑only demonstration of Bowens QGG for external review. Internal engine mechanics remain sealed. This package shows uplift behavior, replay fidelity, anomaly detection, and cross‑domain stability using representative demo outputs.

2. Uplift DemonstrationDataset: Synthetic Calibration Set ABaseline SNR: 14.2QGG Uplifted SNR: 19.8ΔSNR: +5.6

Baseline Structural Coherence: 0.71QGG Structural Coherence: 0.89ΔCoherence: +0.18

Baseline Feature Stability: 0.83QGG Feature Stability: 0.97ΔStability: +0.14

3. Replay Fidelity DemonstrationCycle: #12Replay Fidelity: 0.9921Replay Drift: 0.0030Variance Across 10 Replays: 0.0008

Replay Hash:b54c9f2a7e1d44c0a8f3e91d0c2f7e9a

4. Anomaly Detection DemonstrationAnomaly ID: QKD_fidelity_sag_burst_lossDetected Fidelity Dip: 0.947Burst Loss Window: 3.2 msSeverity: ModerateReproducible: Yes

Replay Hash:e91d77ac4b2f0c3d9a55f1e0c9b2d44f

5. Cross‑Domain Stability DemonstrationDomains Tested:- Astrophysical synthetic- ISR low‑SNR- Calibration grid- Gravitational waveform synthetic

Observed Stability:- Variance ≤ 1% across all domains- No catastrophic drift- No domain‑specific tuning required

6. Reviewer Evaluation NotesThis demo package is intended for evaluation of uplift behavior, reproducibility, anomaly detection, cross‑domain stability, and sealed artifact lineage. Internal logic and operator mechanics remain sealed.

7. CitationBowens QGG — Zenodo Demo Package (External Review Edition)Author: Earl BowensVersion: External Review EditionYear: 2025
DOI: 10.5281/zenodo.18087651
title: Amplified thermal hysteresis of Re during European heatwaves

description: This repository contains the datasets used in the research article "Phase-asymmetric thermal sensitivity amplifies respiration hysteresis in heatwaves". This repository contains site-level flux data and CLM5 simulation data under normal and heatwave conditions.
DOI: 10.5281/zenodo.18087652
title: Amplified thermal hysteresis of Re during European heatwaves

description: This repository contains the datasets used in the research article "Phase-asymmetric thermal sensitivity amplifies respiration hysteresis in heatwaves". This repository contains site-level flux data and CLM5 simulation data under normal and heatwave conditions.
DOI: 10.15468/dl.9j2q9c
title: Occurrence Download

description: A dataset containing 49 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Continent is Asia",
 "Country is China",
 "HasCoordinate is true",
 "HasGeospatialIssue is false",
 "TaxonKey is Alisma gramineum"
 ]
}

 The dataset includes 49 records from 4 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068631-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.j6jnaw
title: Occurrence Download

description: A dataset containing 67 species occurrences available in GBIF matching the query:
{
 "and" : [
 {
 "or" : [
 "PublishingCountry is one of (Argentina, Falkland Islands (Malvinas), South Georgia and the South Sandwich Islands)",
 {
 "and" : [
 "Country is one of (Argentina, Falkland Islands (Malvinas), South Georgia and the South Sandwich Islands)",
 "HasGeospatialIssue is false"
 ]
 },
 "Geometry POLYGON((-74 -60, -25 -60, -25 -90, -74 -90, -74 -60))"
 ]
 },
 {
 "and" : [
 "TaxonKey is one of (Xolmis rubetra [GBIF Backbone Taxonomy])",
 "StateProvince is one of (Buenos Aires)"
 ]
 }
 ]
}

 The dataset includes 67 records from 4 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068632-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/dl.hfm7nq
title: Occurrence Download

description: A dataset containing 5 species occurrences available in GBIF matching the query:
{
 "TaxonKey" : [
 "is Tylototriton thaiorum"
 ]
}

 The dataset includes 5 records from 2 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068633-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.5281/zenodo.18058644
title: Supporting Data for Chaves et al. (2026): Impact of mantle velocity uncertainty on receiver-function imaging of the transition zone

description: This repository contains the data products and codes used in the study “Impact of mantle velocity uncertainty on receiver-function imaging of the transition zone,” submitted to Geophysical Research Letters.

The repository includes codes for simulations using two global mantle tomography models: S40RTS (Ritsema et al., 2011) and GLAD-M35 (Cui et al., 2024). Together with the provided archive CMTFILES_RF_SIMULATIONS.tar.bz2, the packagesspecfem3d_globe7_GLADM35S_GLADM35P_nocrust_stations_1x1_RF_8s_01.tar.bz2 andspecfem3d_globe7_S40RTS_nocrust_stations_1x1_RF_8s_01.tar.bz2are preconfigured to generate the synthetic seismograms used for the receiver-function analysis. The file with our array of stations (STATIONS) is already in the code files, within the folder DATA. 

These synthetic seismograms are used to evaluate how uncertainties in mantle seismic velocities affect imaging of the 400-km and 670-km discontinuities in the mantle transition zone.

The script script_processing.csh documents all processing parameters applied to the synthetic waveforms and reproduces the figures presented in the manuscript.

Output parameters

The tables within the files TABLES_S40RTS.tar.bz2 and TABLES_GLADM35.tar.bz2 were generated by the script script_processing.csh and contain the following header and parameters:





cp_lat (degree) – Latitude of the cap center




cp_lon (degree) – Longitude of the cap center




cp_rad (degree) – Radius of the cap




P–P400s (s) – Time difference between the P arrival (centered at 0 s) and the P400s phase, picked at maximum amplitude




T_ref_P–P400s (s) – Reference P–P400s time at an epicentral distance of 67°




dt_P–P400s (s) – Travel-time residual (P–P400s minus T_ref_P–P400s)




A_P400s / A_P – Amplitude ratio between P400s and P




P–P670s (s) – Time difference between the P arrival (centered at 0 s) and the P670s phase, picked at maximum amplitude




T_ref_P–P670s (s) – Reference P–P670s time at an epicentral distance of 67°




dt_P–P670s (s) – Travel-time residual (P–P670s minus T_ref_P–P670s)




A_P670s / A_P – Amplitude ratio between P670s and P




depth_400 (km) – Depth of the 400-km discontinuity inferred from P–P400s




delta_depth_P400 (km) – Deviation from the nominal 400-km depth




depth_670 (km) – Depth of the 670-km discontinuity inferred from P–P670s




delta_depth_P670 (km) – Deviation from the nominal 670-km depth
DOI: 10.5281/zenodo.18058645
title: Supporting Data for Chaves et al. (2026): Impact of mantle velocity uncertainty on receiver-function imaging of the transition zone

description: This repository contains the data products and codes used in the study “Impact of mantle velocity uncertainty on receiver-function imaging of the transition zone,” submitted to Geophysical Research Letters.

The repository includes codes for simulations using two global mantle tomography models: S40RTS (Ritsema et al., 2011) and GLAD-M35 (Cui et al., 2024). Together with the provided archive CMTFILES_RF_SIMULATIONS.tar.bz2, the packagesspecfem3d_globe7_GLADM35S_GLADM35P_nocrust_stations_1x1_RF_8s_01.tar.bz2 andspecfem3d_globe7_S40RTS_nocrust_stations_1x1_RF_8s_01.tar.bz2are preconfigured to generate the synthetic seismograms used for the receiver-function analysis. The file with our array of stations (STATIONS) is already in the code files, within the folder DATA. 

These synthetic seismograms are used to evaluate how uncertainties in mantle seismic velocities affect imaging of the 400-km and 670-km discontinuities in the mantle transition zone.

The script script_processing.csh documents all processing parameters applied to the synthetic waveforms and reproduces the figures presented in the manuscript.

Output parameters

The tables within the files TABLES_S40RTS.tar.bz2 and TABLES_GLADM35.tar.bz2 were generated by the script script_processing.csh and contain the following header and parameters:





cp_lat (degree) – Latitude of the cap center




cp_lon (degree) – Longitude of the cap center




cp_rad (degree) – Radius of the cap




P–P400s (s) – Time difference between the P arrival (centered at 0 s) and the P400s phase, picked at maximum amplitude




T_ref_P–P400s (s) – Reference P–P400s time at an epicentral distance of 67°




dt_P–P400s (s) – Travel-time residual (P–P400s minus T_ref_P–P400s)




A_P400s / A_P – Amplitude ratio between P400s and P




P–P670s (s) – Time difference between the P arrival (centered at 0 s) and the P670s phase, picked at maximum amplitude




T_ref_P–P670s (s) – Reference P–P670s time at an epicentral distance of 67°




dt_P–P670s (s) – Travel-time residual (P–P670s minus T_ref_P–P670s)




A_P670s / A_P – Amplitude ratio between P670s and P




depth_400 (km) – Depth of the 400-km discontinuity inferred from P–P400s




delta_depth_P400 (km) – Deviation from the nominal 400-km depth




depth_670 (km) – Depth of the 670-km discontinuity inferred from P–P670s




delta_depth_P670 (km) – Deviation from the nominal 670-km depth
DOI: 10.15468/dl.3xja5z
title: Occurrence Download

description: A dataset containing 2765 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is Nepal",
 "TaxonKey is Gyps bengalensis",
 "Year 1000-2025"
 ]
}

 The dataset includes 2765 records from 9 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068634-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.48322/y8gb-3n29
title: PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V1-V2 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data

description: PSP FIELDS Digital Fields Board, DFB, dV12 data:

The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].

DFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The frequency response curves for these bins are given in [3].

The Level 2 data products contained in this data file have been calibrated for:

* 1) The ~6.3 dB loss associated with forming the bandpass signal, see reference [3]
* 2) DFB in-band gain
* 3) The search coil preamplifier response, when applicable

Calibrations for the DFB digital filter gains and analog filter gains have not been implemented as it was determined that these could not be applied accurately to single numerical values representing a broadband signal response and because all bins except the highest frequency bin have a flat gain response equal to one due to these filters. Calibrations for the FIELDS preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.

The Level 2 data products contained in this data file are expressed in sensor coordinates: e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.

The time resolution of the DFB AC bandpass filtered data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB AC bandpass filtered data cadence is typically 1/8 of a NYsecond [2]. Timestamps correspond to the center time of each window.

References:

* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116
* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445
* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344
DOI: 10.48322/ydvh-f703
title: PSP FIELDS Antenna Electronics Board (AEB) Housing Keeping Data

description: PSP FIELDS Antenna Electronics Board (AEB) Housing Keeping Data.
DOI: 10.48322/6nn3-ts64
title: PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V3-V4 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data

description: PSP FIELDS Digital Fields Board, DFB, dV34 data:

The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].

DFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The frequency response curves for these bins are given in [3].

The Level 2 data products contained in this data file have been calibrated for:

* 1) The ~6.3 dB loss associated with forming the bandpass signal, see reference [3]
* 2) DFB in-band gain
* 3) The search coil preamplifier response, when applicable

Calibrations for the DFB digital filter gains and analog filter gains have not been implemented as it was determined that these could not be applied accurately to single numerical values representing a broadband signal response and because all bins except the highest frequency bin have a flat gain response equal to one due to these filters. Calibrations for the FIELDS preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.

The Level 2 data products contained in this data file are expressed in sensor coordinates: e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.

The time resolution of the DFB AC bandpass filtered data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB AC bandpass filtered data cadence is typically 1/8 of a NYsecond [2]. Timestamps correspond to the center time of each window.

References:

* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116
* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445
* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344
DOI: 10.48322/6svt-vr86
title: PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer, SCM, Bandpass filtered, Low Frequency, High Gain, u-component, Sensor coordinates, Level 2 (L2), 0.873813 s Data

description: PSP FIELDS Digital Fields Board, DFB, SCMulfhg data:

The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].

DFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The frequency response curves for these bins are given in [3].

The Level 2 data products contained in this data file have been calibrated for:

* 1) The ~6.3 dB loss associated with forming the bandpass signal, see reference [3]
* 2) DFB in-band gain
* 3) The search coil preamplifier response, when applicable

Calibrations for the DFB digital filter gains and analog filter gains have not been implemented as it was determined that these could not be applied accurately to single numerical values representing a broadband signal response and because all bins except the highest frequency bin have a flat gain response equal to one due to these filters. Calibrations for the FIELDS preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.

The Level 2 data products contained in this data file are expressed in sensor coordinates: e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.

The time resolution of the DFB AC bandpass filtered data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB AC bandpass filtered data cadence is typically 1/8 of a NYsecond [2]. Timestamps correspond to the center time of each window.

References:

* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116
* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445
* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344
DOI: 10.48322/be3k-1d62
title: PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer, SCM, Bandpass filtered, Medium Frequency, High Gain, u-component, Sensor coordinates, Level 2 (L2), 0.873813 s Data

description: PSP FIELDS Digital Fields Board, DFB, SCMumfhg data:

The DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].

DFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The frequency response curves for these bins are given in [3].

The Level 2 data products contained in this data file have been calibrated for:

* 1) The ~6.3 dB loss associated with forming the bandpass signal, see reference [3]
* 2) DFB in-band gain
* 3) The search coil preamplifier response, when applicable

Calibrations for the DFB digital filter gains and analog filter gains have not been implemented as it was determined that these could not be applied accurately to single numerical values representing a broadband signal response and because all bins except the highest frequency bin have a flat gain response equal to one due to these filters. Calibrations for the FIELDS preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.

The Level 2 data products contained in this data file are expressed in sensor coordinates: e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.

The time resolution of the DFB AC bandpass filtered data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB AC bandpass filtered data cadence is typically 1/8 of a NYsecond [2]. Timestamps correspond to the center time of each window.

References:

* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116
* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445
* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344