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2 results for “solar spectrum”

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zenodo48/100

Atlas of the Solar Intensity Spectrum and its Center-to-Limb Variation

<p>The atlas of the Third Solar Spectrum (SS3) represents the ratio between the intensity spectrum at different distances from the solar limb and the intensity spectrum at disk center (&micro; = 1.0), both in units of the intensity of the local continuum level.&nbsp; The observed positions of the measurements cover 9 different &micro; values along the solar axis ranging from 0.1 to 0.9 in step of 0.1, where&nbsp; &micro;=cos&theta; is the cosine&nbsp; of the heliocentric angle &theta;. The current version of the atlas covers the range 4384- 6610 &Aring;.</p> <p>In the PDF file, the first plot represents the spectrum at the center of the solar disk, recorded at IRSOL. The next 9 plots represent the 3rd solar spectrum for &micro;=0.1, &micro;=0.2, &micro;=0.3, &hellip;, &micro;=0.9</p> <p>Columns of the CSV file:</p> <table> <tbody> <tr> <td><strong>WL:</strong></td> <td>Wavelength, 4384-6610 &Aring;</td> </tr> <tr> <td><strong>IC:</strong></td> <td>I/I<sub>c</sub> at disc center</td> </tr> <tr> <td><strong>RMU01:</strong></td> <td>limb / disk-center ratio at &micro;=0.1</td> </tr> <tr> <td><strong>RMU02:</strong></td> <td>limb / disk-center ratio at &micro;=0.2</td> </tr> <tr> <td><strong>&hellip;</strong></td> <td>&hellip;</td> </tr> <tr> <td><strong>RMU09:</strong></td> <td>limb / disk-center ratio at &micro;=0.9</td> </tr> </tbody> </table>

opencc-by-4.0Aug 2017View details →
zenodo48/100

Solar and interplanetary magnetic field data analyzed in "Optimal frequency-domain analysis for spacecraft time series: Introducing the missing-data multitaper power spectrum estimator"

<p>This dataset contains simultaneous measurements of the interplanetary magnetic field magnitude &lt;B&gt;&nbsp;and the sun&#39;s radio flux at 10.7 cm &lt;F10.7&gt;. &lt;B&gt; measurements&nbsp;come from a series of spacecraft located at the L1 point, while&nbsp;&lt;F10.7&gt; was measured by the ongoing monitoring program by&nbsp;Canada&#39;s Dominion Radio Astrophysical Observatory. Bartels rotation-averaged data&nbsp;were downloaded from&nbsp;NASA&#39;s OMNIWeb,&nbsp;https://omniweb.gsfc.nasa.gov/html/ow_data.html. The file contains&nbsp;other solar wind plasma parameters that were not used in the analysis.</p>

opencc-by-4.0Jun 2023View details →

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