adsabs/AstroCLIMB huggingface dataset:
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Map of DAS and colocated seismometers and infrasound instruments deployed at two sites: at the Eureka Airport (left) and in Newark Valley (right). OREXA, OREXB, OREXC, OREXD, OREXE, and OREXF are colocated seismometer/infrasound pairs. DAS IU(s) indicates the DAS interrogator unit(s). At the Eureka Airport, fiber was placed running from the DAS IU toward OREXC and continuing along the edge of the main taxi runway, before bending 90° toward the west (toward OREXB) along the cross runway, then returning to the main taxiway and continuing north toward OREXA. The fiber returned from the turnaround point to the north of OREXA and continued directly toward OREXC without returning to OREXB. In Newark Valley, the fiber ran from the DAS IU south past OREXD, OREXE, and OREXF. A spool with the remaining fiber was placed near OREXF.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Left: AWE’s PSDJK array. Right: LANL’s OREX1 array. Panels top to bottom show values of apparent velocity (Vapp), back azimuth (Baz), and F-statistic (F) corresponding to the beam direction that exhibits the highest signal coherence across consecutive 4 s long windows (overlapping by 50%). Orange circles represent time periods for which there is a >95% probability that the window contains a signal with an SNR greater than or equal to 4. The bottom panel shows the 1–4 Hz beam for a back azimuth of approximately 345°. Note that the OSIRIS-REx signal is seen above a persistent low-SNR signal arriving from a back azimuth of approximately 260°.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Comparison of pressure and ground velocity data at the central elements of the (a) western and (b) eastern UM seismoacoustic arrays. Pressure and velocity amplitude values are provisional pending further calibration of the instruments. Time is relative to 14:45:13.818 UTC. (c) Vertical velocity waveforms from the Golay 3 × 6 array plotted as a function of distance from an azimuth of 0°, i.e., the data have been plotted along a virtual north–south profile, with north at the top of the figure. Waveform amplitudes have been normalized. Note the large oscillating secondary arrivals for stations in the south. Time is relative to 14:45:13.818 UTC.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: High-SNR arrivals on the colocated OREXF infrasound (top) and three-channel seismic (middle) sensors and on fiber wrapped around a spool near OREXF (bottom); the sensor is at 7436 m from the interrogator at channel 3718. Data are filtered with a bandpass filter from [1–10] Hz for the infrasound channel, [2–35] Hz for the seismic channels, and [3–50] Hz for the DAS channel. Time picks are shown with open circles.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Left panel: time trace from the four Chaparral Physics model 64 s sensors in OSU Array 1 located at the Wendover Airport. Right panel: satellite image showing the orientation of the sensors (Chap 1–4), with colors matching those in the left panel, which shows that the signal was arriving from the south–southeast direction. The width across the map is 175 m.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Example infrasound balloon configuration from the OSIRIS-REx deployment. This is the low-altitude weather balloon just after release. Photo credit: R. Lewis.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Signals received at Gem stations situated south of the nominal reentry path in Newark Valley (Strawberry Road). The time series were filtered (high pass, 10 s). The x-axis is in seconds from 14:45:50 UTC.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Signal detected at one of the TDA sensors of the Large N-array. The strong signal is clearly visible just before the 400 s mark. The top panel shows the time series, while the bottom panel shows the spectrogram.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Geometry and response of the Golay 3 × 6 Array. (a) The OSIRIS-REx array design. (b) The co-array, which consists of distances and azimuths between all pairs of stations of the array. (c) The broadband array response for a vertically incident plane wave for the frequency band 0.25–35 Hz.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Signal detection at the West Wendover Airport, Utah. The time series in the bottom panel shows the smartphone microphone equivalent high-pass filter response of the N-wave; the time between the two distinct peaks is the N-wave duration. The top panel shows the multiresolution time-frequency representation of the signal using a Stockwell transform (Garces 2023) and showing the lower-frequency components of the N-wave. All channels of the Wendover array showed nearly identical waveforms time-shifted by their arrival time.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: University of Memphis seismoacoustic array experiment. Yellow triangles show the location of the three-component seismic nodes in the Golay 3 × 6 array configuration (A1–A18). Red triangles show the center infrasound instrument and colocated three-component seismic node for the western and eastern infrasound arrays (A19 + IW1, A20 + IE1). Green triangles show locations for infrasound microphones. Green lines show locations for the P and SH refraction profiles near the western and eastern infrasound arrays. The red lines show the boundary of the airport property.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: Detections made by smartphones, ordered by arrival time. The arrival waveforms and spectra are similar to those in Figure A13, but the N-wave duration depends on the source height and speed. The timing of the arrivals corresponds to the time of closest approach of the source plus the time it would take to reach the station. This arrival pattern is only possible from hypersonic and supersonic sources.
Paper: Geophysical Observations of the 2023 September 24 OSIRIS-REx Sample Return Capsule Reentry
Authors: Elizabeth A. Silber, Daniel C. Bowman, Chris G. Carr, David P. Eisenberg, Brian R. Elbing, Benjamin Fernando, Milton A. Garcés, Robert Haaser, Siddharth Krishnamoorthy, Charles A. Langston, Yasuhiro Nishikawa, Jeremy Webster, Jacob F. Anderson, Stephen Arrowsmith, Sonia Bazargan, Luke Beardslee, Brant Beck, Jordan W. Bishop, Philip Blom, Grant Bracht, David L. Chichester, Anthony Christe, Jacob Clarke, Kenneth Cummins, James Cutts, Lisa Danielson, Carly Donahue, Kenneth Eack, Michael Fleigle, Douglas Fox, Ashish Goel, David Green, Yuta Hasumi, Chris Hayward, Dan Hicks, Jay Hix, Stephen Horton, Emalee Hough, David P. Huber, Madeline A. Hunt, Jennifer Inman, S. M. Ariful Islam, Jacob Izraelevitz, Jamey D. Jacob, James Johnson, Real J. KC, Attila Komjathy, Eric Lam, Justin LaPierre, Kevin Lewis, Richard D. Lewis, Patrick Liu, Léo Martire, Meaghan McCleary, Elisa A. McGhee, Ipsita Mitra, Amitabh Nag, Luis Ocampo Giraldo, Karen Pearson, Mathieu Plaisir, Sarah K. Popenhagen, Hamid Rassoul, Miro Ronac Giannone, Mirza Samnani, Nicholas Schmerr, Kate Spillman, Girish Srinivas, Samuel K. Takazawa, Alex Tempert, Reagan Turley, Cory Van Beek, Loïc Viens, Owen A. Walsh, Nathan Weinstein, Robert White, Brian Williams, Trevor C. Wilson, Shirin Wyckoff, Masa-yuki Yamamoto, Zachary Yap, Tyler Yoshiyama, Cleat Zeiler
Figure caption: (a) Picture of one of the windscreen boxes (Swaim et al. 2023) that housed a GEM sensor. (b) View from above with the cover removed showing a single GEM sensor held within an enclosure and positioned within the windscreen box (photo credit: B. Elbing).