Zobrazeno 1 - 10
of 223
pro vyhledávání: '"Gosain, S."'
Autor:
Gopalswamy, N., Christe, S., Fung, S. F., Gong, Q., Gruesbeck, J. R., Jian, L. K., Kanekal, S. G., Kay, C., Kucera, T. A., Leake, J. E., Li, L., Makela, P., Nikulla, P., Reginald, N. L., Shih, A., Tadikonda, S. K., Viall, N., Wilson III, L. B., Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A. C., Winebarger, A. R., DeForest, C., Hassler, D. M., Seaton, D. B., Desai, M. I., Mokashi, P. S., Lazio, J., Jensen, E. A., Manchester, W. B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D. B., Bale, S. D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G. J. D., Pevtsov, A., Tripathy, S. C., Zhao, J., Scherrer, P. H., Rajaguru, S. P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K. S., Park, Y. D., Jackson, B. V.
We report on a study of the Multiview Observatory for Solar Terrestrial Science (MOST) mission that will provide comprehensive imagery and time series data needed to understand the magnetic connection between the solar interior and the solar atmosphe
Externí odkaz:
http://arxiv.org/abs/2303.02895
Autor:
Pevtsov, Alexei A., Woods, T., Martinez-Pillet, V., Hassler, D., Berger, T., Gosain, S., Hoeksema, T., Jones, A. R., Kohnert, R., Chen, T. Y., Upton, L., Pulkkinen, A.
This White Paper argues for the urgent need for the multi-vantage/multi-point observations of the Sun and the heliosphere in the framework of six (6) key science objectives. We further emphasize the critical importance of 5D-``space'': three spatial,
Externí odkaz:
http://arxiv.org/abs/2211.06715
Autor:
Pevtsov, Alexei A., Martinez-Pillet, V., Gilbert, H., de Wijn, A. G., Roth, M., Gosain, S., Upton, L. A., Katsukawa, Y., Burkepile, J., Zhang, Jie, Reardon, K. P., Bertello, L., Jain, K., Tripathy, S. C., Leka, K. D.
Long-term synoptic observations of the Sun are critical for advancing our understanding of Sun as an astrophysical object, understanding the solar irradiance and its role in solar-terrestrial climate, for developing predictive capabilities of solar e
Externí odkaz:
http://arxiv.org/abs/2211.06712
Autor:
Bertello, L., Arge, N., De Wijn, A. G., Gosain, S., Henney, C., Leka, K. D., Linker, J., Liu, Y., Luhmann, J., Macniece, P. J., Petrie, G., Pevtsov, A., Pevtsov, A. A.
This white paper advocates the importance of multi-height measurements of the vector magnetic field in the solar atmosphere. As briefly described in this document, these measurements are critical for addressing some of the most fundamental questions
Externí odkaz:
http://arxiv.org/abs/2209.04453
Autor:
Gopalswamy, N., Christe, S., Fung, S.F., Gong, Q., Gruesbeck, J.R., Jian, L.K., Kanekal, S.G., Kay, C., Kucera, T.A., Leake, J.E., Li, L., Mӓkelӓ, P., Nikulla, P., Reginald, N.L., Shih, A., Tadikonda, S.K., Viall, N., Wilson, L.B., III, Yashiro, S., Golub, L., DeLuca, E., Reeves, K., Sterling, A.C., Winebarger, A.R., DeForest, C., Hassler, D.M., Seaton, D.B., Desai, M.I., Mokashi, P.S., Lazio, J., Jensen, E.A., Manchester, W.B., Sachdeva, N., Wood, B., Kooi, J., Hess, P., Wexler, D.B., Bale, S.D., Krucker, S., Hurlburt, N., DeRosa, M., Gosain, S., Jain, K., Kholikov, S., Petrie, G.J.D., Pevtsov, A., Tripathy, S.C., Zhao, J., Scherrer, P.H., Rajaguru, S.P., Woods, T., Kenney, M., Zhang, J., Scolini, C., Cho, K.-S., Park, Y.-D., Jackson, B.V.
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics January 2024 254
Present day solar imaging spectrometers typically yield a few hundred million spectra in one hour of observing time. This number will increase by an order of magnitude for future instruments with larger 4k x 4k sensors as planned to be used for the u
Externí odkaz:
http://arxiv.org/abs/1904.11843
High-resolution imaging spectroscopy in solar physics has relied on Fabry-Perot Interferometers (FPIs) in recent years. FPI systems, however, get technically challenging and expensive for telescopes larger than the 1-m class. A conventional slit spec
Externí odkaz:
http://arxiv.org/abs/1712.07077
Solar eruptive phenomena, like flares and coronal mass ejections(CMEs) are governed by magnetic fields. To describe the structure of these phenomena one needs information on the magnetic flux density and the electric current density vector components
Externí odkaz:
http://arxiv.org/abs/1310.5790
The magnetic field permeating the solar atmosphere is generally thought to provide the energy for much of the activity seen in the solar corona, such as flares, coronal mass ejections (CMEs), etc. To overcome the unavailability of coronal magnetic fi
Externí odkaz:
http://arxiv.org/abs/1309.5853
We use daily full-disk vector magnetograms from Vector Spectromagnetograph (VSM) on Synoptic Optical Long-term Investigations of the Sun (SOLIS) system to synthesize the first Carrington maps of the photospheric vector magnetic field. We describe the
Externí odkaz:
http://arxiv.org/abs/1305.3294