The Solar eruptioN Integral Field Spectrograph
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arXiv
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| Autori principali: | , , , , , , , , , , , , , , , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| author | Herde, Vicki L. Chamberlin, Phillip C. Schmit, Don Daw, Adrian Milligan, Ryan O. Polito, Vanessa Bose, Souvik Boyajian, Spencer Buedel, Paris Edgar, Will Gebben, Alex Gong, Qian Jacobsen, Ross Nell, Nicholas Schwab, Bennet Sims, Alan Summers, David Turner, Zachary Valade, Trace Wallace, Joseph |
| author_facet | Herde, Vicki L. Chamberlin, Phillip C. Schmit, Don Daw, Adrian Milligan, Ryan O. Polito, Vanessa Bose, Souvik Boyajian, Spencer Buedel, Paris Edgar, Will Gebben, Alex Gong, Qian Jacobsen, Ross Nell, Nicholas Schwab, Bennet Sims, Alan Summers, David Turner, Zachary Valade, Trace Wallace, Joseph |
| contents | The Solar eruptioN Integral Field Spectrograph (SNIFS) is a solar-gazing spectrograph scheduled to fly in the summer of 2025 on a NASA sounding rocket. Its goal is to view the solar chromosphere and transition region at a high cadence (1s) both spatially (0.5") and spectrally (33 mÅ) viewing wavelengths around Lyman Alpha (1216 Å), Si iii (1206 Å) and O v (1218 Å) to observe spicules, nanoflares, and possibly a solar flare. This time cadence will provide yet-unobserved detail about fast-changing features of the Sun. The instrument is comprised of a Gregorian-style reflecting telescope combined with a spectrograph via a specialized mirrorlet array that focuses the light from each spatial location in the image so that it may be spectrally dispersed without overlap from neighboring locations. This paper discusses the driving science, detailed instrument and subsystem design, and pre-integration testing of the SNIFS instrument. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_08834 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The Solar eruptioN Integral Field Spectrograph Herde, Vicki L. Chamberlin, Phillip C. Schmit, Don Daw, Adrian Milligan, Ryan O. Polito, Vanessa Bose, Souvik Boyajian, Spencer Buedel, Paris Edgar, Will Gebben, Alex Gong, Qian Jacobsen, Ross Nell, Nicholas Schwab, Bennet Sims, Alan Summers, David Turner, Zachary Valade, Trace Wallace, Joseph Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Space Physics The Solar eruptioN Integral Field Spectrograph (SNIFS) is a solar-gazing spectrograph scheduled to fly in the summer of 2025 on a NASA sounding rocket. Its goal is to view the solar chromosphere and transition region at a high cadence (1s) both spatially (0.5") and spectrally (33 mÅ) viewing wavelengths around Lyman Alpha (1216 Å), Si iii (1206 Å) and O v (1218 Å) to observe spicules, nanoflares, and possibly a solar flare. This time cadence will provide yet-unobserved detail about fast-changing features of the Sun. The instrument is comprised of a Gregorian-style reflecting telescope combined with a spectrograph via a specialized mirrorlet array that focuses the light from each spatial location in the image so that it may be spectrally dispersed without overlap from neighboring locations. This paper discusses the driving science, detailed instrument and subsystem design, and pre-integration testing of the SNIFS instrument. |
| title | The Solar eruptioN Integral Field Spectrograph |
| topic | Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics Instrumentation and Detectors Space Physics |
| url | https://arxiv.org/abs/2407.08834 |