Zobrazeno 1 - 10
of 141
pro vyhledávání: '"Bisi, M. M."'
Autor:
Temmer, M., Scolini, C., Richardson, I. G., Heinemann, S. G., Paouris, E., Vourlidas, A., Bisi, M. M., teams, writing, Al-Haddad, N., Amerstorfer, T., Barnard, L., Buresova, D., Hofmeister, S. J., Iwai, K., Jackson, B. V., Jarolim, R., Jian, L. K., Linker, J. A., Lugaz, N., Manoharan, P. K., Mays, M. L., Mishra, W., Owens, M. J., Palmerio, E., Perri, B., Pomoell, J., Pinto, R. F., Samara, E., Singh, T., Sur, D., Verbeke, C., Veronig, A. M., Zhuang, B.
The ISWAT clusters H1+H2 have a focus on interplanetary space and its characteristics, especially on the large-scale co-rotating and transient structures impacting Earth. SIRs, generated by the interaction between high-speed solar wind originating in
Externí odkaz:
http://arxiv.org/abs/2308.04851
Autor:
Fallows, R. A., Forte, B., Mevius, M., Brentjens, M. A., Bassa, C. G., Bisi, M. M., Offringa, A., Shaifullah, G., Tiburzi, C., Vedantham, H., Zucca, P.
Publikováno v:
A&A 667, A57 (2022)
Context. The occultation of a radio source by the plasma tail of a comet can be used to probe structure and dynamics in the tail. Such occultations are rare, and the occurrence of scintillation, due to small-scale density variations in the tail, rema
Externí odkaz:
http://arxiv.org/abs/2210.02139
Observations of interplanetary scintillation (IPS - the scintillation of compact radio sources due to density variations in the solar wind) enable the velocity of the solar wind to be determined, and its bulk density to be estimated, throughout the i
Externí odkaz:
http://arxiv.org/abs/2210.02135
Autor:
Liu, Li-Jia, Peng, Bo, Yu, Lei, Yu, Ye-Zhao, Lu, Ji-Guang, Liu, Bin, Chang, O., Bisi, M. M., Collaboration, FAST
Observations of Interplanetary Scintillation (IPS) are an efficient remote-sensing method to study the solar wind and inner heliosphere. From 2016 to 2018, some distinctive observations of IPS sources like 3C 286 and 3C 279 were accomplished with the
Externí odkaz:
http://arxiv.org/abs/2105.02783
Autor:
Zucca, P., Morosan, D. E., Rouillard, A. P., Fallows, R., Gallagher, P. T., Magdalenic, J., Klein, K-L., Mann, G., Vocks, C., Carley, E. P., Bisi, M. M., Kontar, E. P., Rothkaehl, H., Dabrowski, B., Krankowski, A., Anderson, J., Asgekar, A., Bell, M. E., Bentum, M. J., Best, P., Blaauw, R., Breitling, F., Broderick, J. W., Brouw, W. N., Bruggen, M., Butcher, H. R., Ciardi, B., de Geus, E., Deller, A., Duscha, S., Eisloffel, J., Garrett, M. A., Grießmeier, J. M., Gunst, A. W., Heald, G., Hoeft, M., Horandel, J., Iacobelli, M., Juette, E., Karastergiou, A., van Leeuwen, J., McKay-Bukowski, D., Mulder, H., Munk, H., Nelles, A., Orru, E., Paas, H., Pandey, V. N., Pekal, R., Pizzo, R., Polatidis, A. G., Reich, W., Rowlinson, A., Schwarz, D. J., Shulevski, A., Sluman, J., Smirnov, O., Sobey, C., Soida, M., Thoudam, S., Toribio, M. C., Vermeulen, R., van Weeren, R. J., Wucknitz, O., Zarka, P.
Publikováno v:
A&A 615, A89 (2018)
Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be associated with CMEs and reach speeds higher than the local magnetosonic
Externí odkaz:
http://arxiv.org/abs/1804.01025
Autor:
Vocks, C., Mann, G., Breitling, F., Bisi, M. M., Dabrowski, B., Fallows, R., Gallagher, P. T., Krankowski, A., Magdalenic, J., Marque, C., Morosan, D., Rucker, H.
Publikováno v:
A&A 614, A54 (2018)
The quiet solar corona emits meter-wave thermal bremsstrahlung. Coronal radio emission can only propagate above that radius, $R_\omega$, where the local plasma frequency eqals the observing frequency. The radio interferometer LOw Frequency ARray (LOF
Externí odkaz:
http://arxiv.org/abs/1803.00453
Autor:
Morgan, J . S., Macquart, J-P., Ekers, R., Chhetri, R., Tokumaru, M., Manoharan, P. K., Tremblay, S., Bisi, M. M., Jackson, B. V.
We present the first dedicated observations of Interplanetary Scintillation (IPS) with the Murchison Widefield Array (MWA). We have developed a synthesis imaging technique, tailored to the properties of modern "large-N" low-frequency radio telescopes
Externí odkaz:
http://arxiv.org/abs/1709.00312
Autor:
Morosan, D. E., Gallagher, P. T., Fallows, R. A., Reid, H., Mann, G., Bisi, M. M., Magdalenic, J., Rucker, H. O., Thide, B., Vocks, C., Anderson, J., Asgekar, A., Avruch, I. M., Bell, M. E., Bentum, M. J., Best, P., Blaauw, R., Bonafede, A., Breitling, F., Broderick, J. W., Bruggen, M., Cerrigone, L., Ciardi, B., de Geus, E., Duscha, S., Eisloffel, J., Falcke, H., Garrett, M. A., Griessmeier, J. M., Gunst, A. W., Hoeft, M., Iacobelli, M., Juette, E., Kuper, G., McFadden, R., McKay-Bukowski, D., McKean, J. P., Mulcahy, D. D., Munk, H., Nelles, A., Orru, E., Paas, H., Pandey-Pommier, M., Pandey, V. N., Pizzo, R., Polatidis, A. G., Reich, W., Schwarz, D. J., Sluman, J., Smirnov, O., Steinmetz, M., Tagger, M., ter Veen, S., Thoudam, S., Toribio, M. C., Vermeulen, R., van Weeren, R. J., Wucknitz, O., Zarka, P.
Publikováno v:
A&A 606, A81 (2017)
Context. The Sun is an active star that produces large-scale energetic events such as solar flares and coronal mass ejections and numerous smaller-scale events such as solar jets. These events are often associated with accelerated particles that can
Externí odkaz:
http://arxiv.org/abs/1707.03428
Observation of interplanetary scintillation (IPS) beyond Earth-orbit can be challenging due to the necessity to use low radio frequencies at which scintillation due to the ionosphere could confuse the interplanetary contribution. A recent paper by Ka
Externí odkaz:
http://arxiv.org/abs/1608.04504
Autor:
Morosan, D. E., Gallagher, P. T., Zucca, P., O'Flannagain, A., Fallows, R., Reid, H., Magdalenic, J., Mann, G., Bisi, M. M., Kerdraon, A., Konovalenko, A. A., MacKinnon, A. L., Rucker, H. O., Thide, B., Vocks, C., Alexov, A., Anderson, J., Asgekar, A., Avruch, I. M., Bentum, M. J., Bernardi, G., Bonafede, A., Breitling, F., Broderick, J. W., Brouw, W. N., Butcher, H. R., Ciardi, B., de Geus, E., Eisloffel, J., Falcke, H., Frieswijk, W., Garrett, M. A., Griessmeier, J., Gunst, A. W., Hessels, J. W. T., Hoeft, M., Karastergiou, A., Kondratiev, V. I., Kuper, G., van Leeuwen, J., McKay-Bukowski, D., McKean, J. P., Munk, H., Orru, E., Paas, H., Pizzo, R., Polatidis, A. G., Scaife, A. M. M., Sluman, J., Tasse, C., Toribio, M. C., Vermeulen, R., Zarka, P.
Publikováno v:
A&A 580, A65 (2015)
Context. The Sun is an active source of radio emission that is often associated with energetic phenomena ranging from nanoflares to coronal mass ejections (CMEs). At low radio frequencies (<100 MHz), numerous millisecond duration radio bursts have be
Externí odkaz:
http://arxiv.org/abs/1507.07496