Zobrazeno 1 - 10
of 93
pro vyhledávání: '"Kholikov, S."'
Autor:
Tripathy, S. C., Jain, K., Braun, D., Cally, P., Dikpati, M., Felipe, T., Jain, R., Kholikov, S., Khomenko, E., Komm, R., Leibacher, J., Martinez-Pillet, V., Pevtsov, A., Rajaguru, S. P., Roth, M., Uitenbroek, H., Zhao, J.
The goal of helioseismology is to provide accurate information about the Sun's interior from the observations of the wave field at its surface. In the last three decades, both global and local helioseismology studies have made significant advances an
Externí odkaz:
http://arxiv.org/abs/2305.07585
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:
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
We analyze data from the Helioseismic Magnetic Imager (HMI) and the Atmospheric Imaging Assembly (AIA) instruments on board the Solar Dynamics Observatory (SDO) to characterize the spatio-temporal acoustic power distribution in active regions as a fu
Externí odkaz:
http://arxiv.org/abs/1711.01259
Publikováno v:
ApJ, 805, 133 2015
Meridional flow is thought to play a very important role in the dynamics of the solar convection zone; however, because of its relatively small amplitude, precisely measuring it poses a significant challenge. Here we present a complete time-distance
Externí odkaz:
http://arxiv.org/abs/1504.08071
Autor:
Kosovichev, A. G., Basu, S., Bogart, R., Duvall Jr, T. L., Gonzalez-Hernandez, I., Haber, D., Hartlep, T., Howe, R., Komm, R., Kholikov, S., Parchevsky, K. V., Tripathy, S., Zhao, J.
Local helioseismology provides unique information about the subsurface structure and dynamics of sunspots and active regions. However, because of complexity of sunspot regions local helioseismology diagnostics require careful analysis of systematic u
Externí odkaz:
http://arxiv.org/abs/1011.0799
We apply ring-diagram analysis and spherical harmonic decomposition methods to compute 3-dimensional power spectra of magnetograms obtained by the Global Oscillation Network Group (GONG) during quiet periods of solar activity. This allows us to inves
Externí odkaz:
http://arxiv.org/abs/1003.5013
Autor:
Jain, Kiran, Tripathy, S. C., Burtseva, O., Hernandez, I. Gonzalez, Hill, F., Howe, R., Kholikov, S., Komm, R., Leibacher, J.
The availability of continuous helioseismic data for two consecutive solar minima has provided a unique opportunity to study the changes in the solar interior that might have led to this unusual minimum. We present preliminary analysis of inter media
Externí odkaz:
http://arxiv.org/abs/1002.2411
We investigate mode amplitudes in the active and quiet Sun in both maximum and minimum phases of the solar activity cycle. We confirm previous studies showing that p-mode amplitudes at solar minimum are higher than at solar maximum. We mask active re
Externí odkaz:
http://arxiv.org/abs/0904.0440
We study variations of the lifetimes of high-degree solar p-modes in the quiet and active Sun with the solar activity cycle. The lifetimes in the degree range 300 - 600 and frequency 2.5 - 4.5 mHz were computed from SOHO/MDI data in an area including
Externí odkaz:
http://arxiv.org/abs/0902.2016