Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data
As first discussed by Farrugia et al. (J. Geophys. Res., 103, 6543, 1998), coronal mass ejections (CMEs) may support the excitation of electromagnetic ion cyclotron waves (EICWs). The proton plasma beta, and the electron temperature and anisotropy in the front region (~5 hours, translating to ~6×106...
Guardado en:
| Autor principal: | |
|---|---|
| Otros Autores: | , , , , |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2001
|
| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 05840caa a22007337a 4500 | ||
|---|---|---|---|
| 001 | PAPER-1864 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250424085852.0 | ||
| 008 | 190411s2001 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0035655249 | |
| 030 | |a ASRSD | ||
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Dasso, Sergio Ricardo | |
| 245 | 1 | 0 | |a Waves in the proton cyclotron frequency range in the CME observed by wind on August 7-8,1996: Theory and data |
| 260 | |c 2001 | ||
| 270 | 1 | 0 | |m Dasso, S.; Instituto de Fisica del Plasma, CONICET - FCENyN/UBA, Buenos Aires, Argentina |
| 504 | |a Burlaga, L.F., Sittler, E., Mariani, F., Schwenn, R., (1981) J. Geophys. Res, 86, p. 6673 | ||
| 504 | |a Burlaga, L.F., (1995) Interplanetary Magnetohydrodynamics, , Oxford Univ. Press, New York | ||
| 504 | |a Dasso, S., Gratton, F.T., Farrugia, C.J., Gnavi, G., (1998) Proc. VIII Latin American Workshop on Plasma Physics, , Contributed Papers, 111.7-C061, UNCPBA, Tandil, Argentina | ||
| 504 | |a Dasso, S., Gratton, F.T., Farrugia, C.J., Solar wind nine (1999) AIP Conf. Proc, 471, p. 669. , edited by S. Habbal | ||
| 504 | |a Dasso, S., Gratton, F.T., Farrugia, C.J., Gnavi, G., (2000) The Solar Wind-Magnetosphere System, , edited by H.K. Biernat, C.J. Farrugia, and D.F. Vogl, Austrian Academy of Sciences Press, 71, Vienna, Austria | ||
| 504 | |a Farrugia, C.J., Gratton, F.G., Gnavi, G., Ogilvie, K.W., (1998) J. Geophys. Res, 103, p. 6543 | ||
| 504 | |a Galvin, A.B., Ipavich, F.M., Gloeckler, G., Hovestadt, D., Bame, S.J., (1987) J. Geophys. Res, 92, p. 12069 | ||
| 504 | |a Gosling, J.T., Coronal mass ejections and magnetic flux ropes in interplanetary space in Physics of Magnetic Flux Ropes (1990) Geophys. Mongr. Ser, 58, p. 343. , edited by C. T. Russell, E. R. Priest, and L. C. Lee, AGU, Washington, D.C | ||
| 504 | |a Gosling, J.T., Baker, D.N., Bame, S.J., Feldman, W.C., Zwickl, R.D., (1987) J. Geophys. Res, 92, p. 8519 | ||
| 504 | |a Gratton, F.T., Dasso, S., Farrugia, C.J., (1998) Proc. of 1998 Int. Congress on Plasma Physics, 22 C, p. 1122. , Praha, edited by P. Pavlo, ECA, European Physical Society | ||
| 504 | |a Janoo, L., Farrugia, C.J., Torbert, R.B., Quinn, J.M., Szabo, A., (1998) J. Geophys. Res, 103, p. 17249 | ||
| 504 | |a Lopez, R.E., (1987) J. Geophys. Res, 92, p. 11189 | ||
| 504 | |a Osherovich, V.A., Farrugia, C.J., Burlaga, L.F., Lepping, R.P., Fainberg, J., (1993) J. Geophys. Res, 98, p. 15331 | ||
| 504 | |a Richardson, I.G., Cane, H.V., (1995) J. Geophys. Res, 100, p. 23397 | ||
| 504 | |a Richardson, I.C., Farrugia, C.J., Cane, H.V., (1997) J. Geophys. Res, 102, p. 4691 | ||
| 504 | |a Stix, T.H., (1992) Waves in Plasmas, , AIM, New York | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a As first discussed by Farrugia et al. (J. Geophys. Res., 103, 6543, 1998), coronal mass ejections (CMEs) may support the excitation of electromagnetic ion cyclotron waves (EICWs). The proton plasma beta, and the electron temperature and anisotropy in the front region (~5 hours, translating to ~6×106 km) of the CME observed by WIND on August 7-8, 1996 favor this possible excitation. Supplementing these measured parameters by other data taken from a survey of CME properties observed by the ISEE 3 spacecraft (Gosling et al., J. Geophys. Res., 92, 8519, 1987), we solve the EICW dispersion relation numerically. We find short e-folding times of EICWs, of the order of 5 min, i.e., much less than the typical evolution time of these ejecta. We suggest that high resolution data will show enhanced power in the 0.5 Hz range. © 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved. |l eng | |
| 536 | |a Detalles de la financiación: PIP 4536/96 | ||
| 536 | |a Detalles de la financiación: Secretaría de Ciencia y Técnica, Universidad de Buenos Aires, TX032/98, X059/2001 | ||
| 536 | |a Detalles de la financiación: NAG5-2834, NAG5-10883 | ||
| 536 | |a Detalles de la financiación: SD thanks to R. Arnoldy and J. Quinn for their hospitality during a research stay at UNH, when part of this work was done. Work supported by USA NASA grant NAG5-2834 and living with a star grant NAG5-10883, and Argentinian grants UBACyT (TX032/98 and X059/2001) and CONICET PIP 4536/96. | ||
| 593 | |a Instituto de Física del Plasma (INFIP), CONICET, FCEyN/UBA, Buenos Aires, Argentina | ||
| 593 | |a Physics Department, FCEyN, UBA, Buenos Aires, Argentina | ||
| 593 | |a Space Science Center, University of New Hampshire, New Hampshire, NH, United States | ||
| 593 | |a NASA, Goddard Space Flight Center, Greenbelt, MD, United States | ||
| 690 | 1 | 0 | |a ANISOTROPY |
| 690 | 1 | 0 | |a SPACE RESEARCH |
| 690 | 1 | 0 | |a SPACECRAFT |
| 690 | 1 | 0 | |a WIND |
| 690 | 1 | 0 | |a ELECTRON TEMPERATURE |
| 690 | 1 | 0 | |a ELECTROMAGNETIC WAVES |
| 690 | 1 | 0 | |a MAGNETOSPHERE |
| 690 | 1 | 0 | |a PLASMA |
| 700 | 1 | |a Farrugia, C.J. | |
| 700 | 1 | |a Gratton, Fausto Tulio Livio | |
| 700 | 1 | |a Lepping, R.P. | |
| 700 | 1 | |a Ogilvie, K.W. | |
| 700 | 1 | |a Fitzenreiter, R.J. | |
| 773 | 0 | |d 2001 |g v. 28 |h pp. 747-752 |k n. 5 |p Adv. Space Res. |x 02731177 |w (AR-BaUEN)CENRE-3577 |t Advances in Space Research | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0035655249&doi=10.1016%2fS0273-1177%2801%2900526-9&partnerID=40&md5=ebdb6e8f6783ad1a5561fcfba085e785 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1016/S0273-1177(01)00526-9 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_02731177_v28_n5_p747_Dasso |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v28_n5_p747_Dasso |y Registro en la Biblioteca Digital |
| 961 | |a paper_02731177_v28_n5_p747_Dasso |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||
| 999 | |c 62817 | ||