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8 results for “STEVE”
Steve Green (g2512)
<b>-- <a href="https://doi.org/10.5281/zenodo.11582199">Documentation</a> --</b><br><br><u>Name</u>: Steve Green<br><u>musiXplora-ID</u>: g2512<br><u>musiXplora-URI</u>: <a href="https://musixplora.de/mxp/g2512">https://musixplora.de/mxp/g2512</a><br><u>Gender</u>: m<br><u>Date of Birth</u>: 1949<br><u>Place of Birth</u>: West Virginia<br><u>Date of Death</u>: 2013<br><u>Place of Death</u>: Undefined<br><u>First Mentioned</u>: 1974<br><u>Sectors</u>: Zupfinstrumentenbau<br><u>Professions (Musical)</u>: Harfenbauer<br><u>Other Places of Activity</u>: USA<br><br><br><u>Portfolio:</u><br><table><tbody><tr><th>Group</th><th>Role</th><th>Name</th><th>mXp-ID</th></tr><tr><td>Sortimente</td><td>Sortiment</td><td>Harfe</td><td><a href="https://musixplora.de/mxp/2001474">2001474</a></td></tr></tbody></table><br><br><u>Changelog</u>:<br> - v0.0.1: Initial Upload.<br>
STEVE images observed on Sept 3rd, 2022, at Athabasca, Canada
<p>These images show the Strong Thermal Emission Velocity Enhancement (STEVE) observed on Sept 3<sup>rd</sup>, 2022, at Athabasca, Canada, using two Nikon D610 cameras with an all-sky fish-eye lens. The two cameras were located at AUGO-I (54.71°N, 246.69°E, C002) and AUGO-II (54.60°N, 246.36°E, C001), respectively. The format of the filename is C00X_YYDDMMhhmmss_0030.jpg.</p>
Under the Stars with Steve, by Sheila Wiwchar, Canada
<p>Third place in the 2021 IAU OAE Astrophotography Contest, category Aurorae (time-lapses).</p> <p>This is a strange atmospheric phenomenon known as Steve. This is similar to an aurora as it is caused by charged particles interacting with the Earth's magnetic field. However unlike aurorae, the particles which cause Steve are generated high in the Earth's atmosphere rather than coming from the Sun. Note the banded "picket fence" appearance. This is caused by waves of these particles in the upper atmosphere. The name Steve was chosen by the first group to describe this phenomenon as a familiar name for something unknown.</p> <p>Sheila Wiwchar/IAU OAE</p>
Morphological Characteristics of STEVE emissions
<p>These photographs of STEVE emissions are captured by two citizen scientists and are in support of the manuscripts to study the magnetospheric driver of STEVE, as well as the morphological characteristics. </p>
Taphozous troughtoní near Mount Isa. Queensland, Australia Photo Steve Parish Lochman Transparencias in Emballonuridae
Taphozous troughtoní near Mount Isa. Queensland, Australia Photo Steve Parish Lochman Transparencias
Letters of Stone: a podcast interview with Steve Robins
<p>A blog entry of an interview conducted with Steve Robins, the writer of the book- Letters of Stone: From Nazi Germany to South Africa (Penguin Books, 2016<br> </p>
data used in "First Observations From the TREx Spectrograph: The Optical Spectrum of STEVE and the Picket Fence Phenomena"
<p>This data was linked in the Acknowledgements of the paper. We upload it to Zenodo for archival preservation.</p>
Raw images used in "Sub-Auroral Green STEVE Arcs – Evidence for Low Energy Excitation"
<p>These are the two raw STEVE images used in the manuscript, included for replicability.</p>
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