Intercomparison of the LASCO-C2, SECCHI-COR1, SECCHI-COR2, and Mk4 Coronagraphs
In order to assess the reliability and consistency of white-light coronagraph measurements, we report on quantitative comparisons between polarized brightness [pB] and total brightness [B] images taken by the following white-light coronagraphs: LASCO-C2 on SOHO, SECCHI-COR1 and -COR2 on STEREO, and...
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| Formato: | Capítulo de libro |
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2012
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 08583caa a22009017a 4500 | ||
|---|---|---|---|
| 001 | PAPER-9376 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518203917.0 | ||
| 008 | 190411s2012 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-84865463165 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Frazin, R.A. | |
| 245 | 1 | 0 | |a Intercomparison of the LASCO-C2, SECCHI-COR1, SECCHI-COR2, and Mk4 Coronagraphs |
| 260 | |c 2012 | ||
| 270 | 1 | 0 | |m Frazin, R. A.; Dept. of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, United States; email: rfrazin@umich.edu |
| 506 | |2 openaire |e Política editorial | ||
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| 504 | |a Zuccarello, F.P., Bemporad, A., Jacobs, C., Mierla, M., Poedts, S., Zuccarello, F., (2012) Astrophys. J., 744, p. 66. , doi:10.1088/0004-637X/744/1/66 | ||
| 520 | 3 | |a In order to assess the reliability and consistency of white-light coronagraph measurements, we report on quantitative comparisons between polarized brightness [pB] and total brightness [B] images taken by the following white-light coronagraphs: LASCO-C2 on SOHO, SECCHI-COR1 and -COR2 on STEREO, and the ground-based MLSO-Mk4. The data for this comparison were taken on 16 April 2007, when both STEREO spacecraft were within 3. 1 {ring operator} of Earth's heliographic longitude, affording essentially the same view of the Sun for all of the instruments. Due to the difficulties of estimating stray-light backgrounds in COR1 and COR2, only Mk4 and C2 produce reliable coronal-hole values (but not at overlapping heights), and these cannot be validated without rocket flights or ground-based eclipse measurements. Generally, the agreement between all of the instruments' pB values is within the uncertainties in bright streamer structures, implying that measurements of bright CMEs also should be trustworthy. Dominant sources of uncertainty and stray light are discussed, as is the design of future coronagraphs from the perspective of the experiences with these instruments. © 2012 Springer Science+Business Media B.V. |l eng | |
| 536 | |a Detalles de la financiación: National Aeronautics and Space Administration, NNX08AJ09G | ||
| 536 | |a Detalles de la financiación: Universidad de Buenos Aires, 20020090100264 | ||
| 536 | |a Detalles de la financiación: Secretaría de Ciencia y Técnica, Universidad de Buenos Aires | ||
| 536 | |a Detalles de la financiación: Centre National d’Etudes Spatiales, CNES | ||
| 536 | |a Detalles de la financiación: University of Michigan, U-M | ||
| 536 | |a Detalles de la financiación: Acknowledgements The authors thank the anonymous referee for helpful comments, which resulted in a much improved manuscript. This research was supported by NASA Heliophysics Guest Investigator award NNX08AJ09G to the University of Michigan. A.M.V. acknowledges UBACyT (Universidad de Buenos Aires) grant no. 20020090100264 for partial financial support. R.J.H. was funded by NASA under GSRP fellowship NNX08AT43H FLL. The LASCO-C2 project at Laboratoire d’Astrophysique de Marseille is funded by the Centre National d’Etudes Spatiales (CNES). The authors thank Katherine Baldwin for her helpful comments. | ||
| 593 | |a Dept. of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI 48109, United States | ||
| 593 | |a Instituto de Astronomía y Física del Espacio, ONICET-UBA and FCEN (UBA), CC 67 - Suc 28, Ciudad de Buenos Aires, Argentina | ||
| 593 | |a Adnet Systems, Inc., NASA Goddard Space Flight Center, Code 671, Greenbelt, MD 20771, United States | ||
| 593 | |a Dept. of Computer Science, University of Illinois, Urbana, IL 61801, United States | ||
| 593 | |a Laboratoire d'Astrophysique de Marseille, UMR6110, CNRS/Université de Provence, 38 rue Frédéric Joliot-Curie, 13388 Marseille Cedex 13, France | ||
| 593 | |a Naval Research Laboratory, Code 7663, Washington, DC 20375, United States | ||
| 593 | |a High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307, United States | ||
| 593 | |a Dept. of Mathematics, Massachusetts Institute of Technology, Cambridge, MA, 02139, United States | ||
| 690 | 1 | 0 | |a CORONAGRAPH |
| 690 | 1 | 0 | |a ELECTRON DENSITY |
| 690 | 1 | 0 | |a SOLAR CORONA |
| 700 | 1 | |a Vásquez, A.M. | |
| 700 | 1 | |a Thompson, W.T. | |
| 700 | 1 | |a Hewett, R.J. | |
| 700 | 1 | |a Lamy, P. | |
| 700 | 1 | |a Llebaria, A. | |
| 700 | 1 | |a Vourlidas, A. | |
| 700 | 1 | |a Burkepile, J. | |
| 773 | 0 | |d 2012 |g v. 280 |h pp. 273-293 |k n. 1 |p Sol. Phys. |x 00380938 |w (AR-BaUEN)CENRE-2238 |t Solar Physics | |
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