The recovery of CME-related dimmings and the ICME's enduring magnetic connection to the Sun
It is generally accepted that transient coronal holes (TCHs, dimmings) correspond to the magnetic footpoints of CMEs that remain rooted in the Sun as the CME expands out into the interplanetary space. However, the observation that the average intensity of the 12 May 1997 dimmings recover to their pr...
Guardado en:
| Autor principal: | |
|---|---|
| Otros Autores: | , , , , , , |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2008
|
| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 12526caa a22013097a 4500 | ||
|---|---|---|---|
| 001 | PAPER-22293 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250618095319.0 | ||
| 008 | 190411s2008 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-55349118465 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Attrill, G.D.R. | |
| 245 | 1 | 4 | |a The recovery of CME-related dimmings and the ICME's enduring magnetic connection to the Sun |
| 260 | |c 2008 | ||
| 270 | 1 | 0 | |m Attrill, G. D. R.; Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom; email: gdra@mssl.ucl.ac.uk |
| 504 | |a Abramenko, V.I., Fisk, L.A., Yurchyshyn, V.B., (2006) Astrophys. J., 641, p. 65 | ||
| 504 | |a Attrill, G., Nakwacki, M.S., Harra, L.K., Van Driel-Gesztelyi, L., Mandrini, C.H., Dasso, S., Wang, J., (2006) Solar Phys., 238, p. 117 | ||
| 504 | |a Attrill, G.D.R., Harra, L.K., Van Driel-Gesztelyi, L., Démoulin, P., Wülser, J.P., (2007) Astron. Nachr., 328, p. 760 | ||
| 504 | |a Baker, D., Van Driel-Gesztelyi, L., Attrill, G.D.R., (2007) Astron. Nachr., 328, p. 773 | ||
| 504 | |a Berger, T.E., De Pontieu, B., Fletcher, L., Schrijver, C.J., Tarbell, T.D., Title, A.M., (1999) Solar Phys., 190, p. 409 | ||
| 504 | |a Burlaga, L., Sittler, E., Mariani, F., Schwenn, R., (1981) J. Geophys. Res., 86, p. 6673 | ||
| 504 | |a Chertok, I.M., Grechnev, V.V., (2003) Astron. Nachr., 47, p. 934 | ||
| 504 | |a Chertok, I.M., Grechnev, V.V., (2005) Solar Phys., 229, p. 95 | ||
| 504 | |a Chertok, I.M., Grechnev, V.V., Hudson, H.S., Nitta, N.V., (2004) J. Geophys. Res., 109, p. 2112. , A18 | ||
| 504 | |a Crooker, N.U., Webb, D.F., (2006) J. Geophys. Res., 111, p. 8108. , A10 | ||
| 504 | |a Crooker, N.U., Gosling, J.T., Kahler, S.W., (2002) J. Geophys. Res., 107, p. 1028 | ||
| 504 | |a Culhane, J.L., Harra, L.K., James, A.M., Al-Janabi, K., Bradley, L.J., Chaudry, R.A., Rees, K., Whillock, M.C.R., (2007) Solar Phys., 243, p. 19 | ||
| 504 | |a De Toma, G., Holzer, T.E., Burkepile, J.T., Gilbert, H.R., (2005) Astrophys. J., 621, p. 1109 | ||
| 504 | |a Delaboudinière, J.P., Artzner, G.E., Brunaud, J., Gabriel, A.H., Hochedez, J.F., Millier, F., Song, X.Y., Howard, R.A., (1995) Solar Phys., 162, p. 291 | ||
| 504 | |a Delannée, C., (2000) Astrophys. J., 545, p. 512 | ||
| 504 | |a Démoulin, P., (2008) Ann. Geophys., , in press | ||
| 504 | |a Fisk, L.A., (2005) Astrophys. J., 626, p. 563 | ||
| 504 | |a Fisk, L.A., Schwadron, N.A., (2001) Astrophys. J., 560, p. 425 | ||
| 504 | |a Fisk, L.A., Zurbuchen, T.H., (2006) J. Geophys. Res., 111, p. 9115. , A10 | ||
| 504 | |a Hagenaar, H.J., Derosa, M.L., Schrijver, C.J., (2008) Astrophys. J., 678, p. 541 | ||
| 504 | |a Hagenaar, H.J., Schrijver, C.J., Title, A.M., Shine, R.A., (1999) Astrophys. J., 511, p. 932 | ||
| 504 | |a Hansen, R.T., Garcia, C.J., Hansen, S.F., Yasukawa, E., (1974) Pub. Astron. Soc. Pac., 86, p. 500 | ||
| 504 | |a Harra, L.K., Sterling, A.C., (2001) Astrophys. J., 561, p. 215 | ||
| 504 | |a Harra, L.K., Crooker, N.U., Mandrini, C.H., Van Driel-Gesztelyi, L., Dasso, S., Wang, J., Elliott, H., Bisi, M.M., (2007) Solar Phys., 244, p. 95 | ||
| 504 | |a Harra, L.K., Hara, H., Imada, S., Young, P., Williams, D.R., Sterling, A.C., Korendyke, C., Attrill, G.D.R., (2007) Pub. Astron. Soc. Japan, 59, p. 801 | ||
| 504 | |a Harrison, R.A., Sawyer, E.C., Carter, M.K., Cruise, A.M., Cutler, R.M., Fludra, A., Hayes, R.W., Parker, D.J., (1995) Solar Phys., 162, p. 233 | ||
| 504 | |a Hudson, H.S., Cliver, E.W., (2001) J. Geophys. Res., 106, p. 25199 | ||
| 504 | |a Hudson, H.S., Acton, L.W., Freeland, S.L., (1996) Astrophys. J., 470, p. 629 | ||
| 504 | |a Imada, S., Hara, H., Watanabe, T., Asai, A., Kamio, S., Matsuzaki, K., Harra, L.K., Mariska, J.T., (2007) Pub. Astron. Soc. Japan, 59, p. 793 | ||
| 504 | |a Jiang, Y., Yang, L., Li, K., Ren, D., (2007) Astrophys. J., 662, p. 131 | ||
| 504 | |a Kahler, S.W., Hudson, H.S., (2001) J. Geophys. Res., 106, p. 29239 | ||
| 504 | |a Khan, J.I., Hudson, H.S., (2000) Geophys. Res. Lett., 27, p. 1083 | ||
| 504 | |a Larson, D.E., Lin, R.P., McTiernan, J.M., McFadden, J.P., Ergun, R.E., McCarthy, M., Rème, H., Lepping, R.P., (1997) Geophys. Res. Lett., 24, p. 1911 | ||
| 504 | |a Lepping, R.P., Acũna, M.H., Burlaga, L.F., Farrell, W.M., Slavin, J.A., Schatten, K.H., Mariani, F., Whang, Y.C., (1995) Space Sci. Rev., 71, p. 207 | ||
| 504 | |a Lin, R.P., Anderson, K.A., Ashford, S., Carlson, C., Curtis, D., Ergun, R., Larson, D., Parks, G.K., (1995) Space Sci. Rev., 71, p. 125 | ||
| 504 | |a Liu, C., Lee, J., Yurchyshyn, V., Deng, N., Cho, K.S., Karlický, M., Wang, H., (2007) Astrophys. J., 669, p. 1372 | ||
| 504 | |a Malandraki, O.E., Lario, D., Lanzerotti, L.J., Sarris, E.T., Geranios, A., Tsiropoula, G., (2005) J. Geophys. Res., 110, pp. 09S06. , A9 | ||
| 504 | |a Mandrini, C.H., Pohjolainen, S., Dasso, S., Green, L.M., Démoulin, P., Van Driel-Gesztelyi, L., Copperwheat, C., Foley, C., (2005) Astron. Astrophys., 434, p. 725 | ||
| 504 | |a Mandrini, C.H., Nakwacki, M.S., Attrill, G., Van Driel-Gesztelyi, L., Démoulin, P., Dasso, S., Elliott, H., (2007) Solar Phys., 244, p. 25 | ||
| 504 | |a Manoharan, P.K., Van Driel-Gesztelyi, L., Pick, M., Demoulin, P., (1996) Astrophys. J., 468, p. 73 | ||
| 504 | |a McComas, D.J., Gosling, J.T., Phillips, J.L., Bame, S.J., Luhmann, J.G., Smith, E.J., (1989) J. Geophys. Res., 94, p. 6907 | ||
| 504 | |a McIntosh, S.W., Leamon, R.J., Davey, A.R., Wills-Davey, M.J., (2007) Astrophys. J., 660, p. 1653 | ||
| 504 | |a Moore, R.L., Sterling, A.C., Hudson, H.S., Lemen, J.R., (2001) Astrophys. J., 552, p. 833 | ||
| 504 | |a Owens, M.J., Crooker, N.U., (2007) J. Geophys. Res., 112, p. 6106 | ||
| 504 | |a Qiu, J., Hu, Q., Howard, T.A., Yurchyshyn, V.B., (2007) Astrophys. J., 659, p. 758. , 10.1086/512060 | ||
| 504 | |a Richardson, I.G., Farrugia, C.J., Burlaga, L.F., (1991) 22nd International Cosmic Ray Conference, 3, p. 597. , Cawley, M., et al. (eds.) | ||
| 504 | |a Riley, P., Gosling, J.T., Crooker, N.U., (2004) Astrophys. J., 608, p. 1100 | ||
| 504 | |a Rust, D.M., (1983) Space Sci. Rev., 34, p. 21 | ||
| 504 | |a Rust, D.M., Hildner, E., (1976) Solar Phys., 48, p. 381 | ||
| 504 | |a Schrijver, C.J., Title, A.M., Van Ballegooijen, A.A., Hagenaar, H.J., Shine, R.A., (1997) Astrophys. J., 487, p. 424 | ||
| 504 | |a Shodhan, S., Crooker, N.U., Kahler, S.W., Fitzenreiter, R.J., Larson, D.E., Lepping, R.P., Siscoe, G.L., Gosling, J.T., (2000) J. Geophys. Res., 105, p. 27261 | ||
| 504 | |a Smith, C.W., L'Heureux, J., Ness, N.F., Acuña, M.H., Burlaga, L.F., Scheifele, J., (1998) Space Sci. Rev., 86, p. 613 | ||
| 504 | |a Sterling, A.C., Hudson, H.S., (1997) Astrophys. J., 491, p. 55 | ||
| 504 | |a Thompson, B.J., Plunkett, S.P., Gurman, J.B., Newmark, J.S., St. Cyr, O.C., Michels, D.J., (1998) Geophys. Res. Lett., 25, p. 2465 | ||
| 504 | |a Thompson, B.J., Cliver, E.W., Nitta, N., Delannée, C., Delaboudinière, J.P., (2000) Geophys. Res. Lett., 27, p. 1431 | ||
| 504 | |a Tsuneta, S., Acton, L., Bruner, M., Lemen, J., Brown, W., Caravalho, R., Catura, R., Owens, J., (1991) Solar Phys., 136, p. 37 | ||
| 504 | |a Vaiana, G.S., Van Speybroeck, L., Zombeck, M.V., Krieger, A.S., Silk, J.K., Timothy, A., (1977) Space Sci. Instr., 3, p. 19 | ||
| 504 | |a Webb, D.F., Lepping, R.P., Burlaga, L.F., Deforest, C.E., Larson, D.E., Martin, S.F., Plunkett, S.P., Rust, D.M., (2000) J. Geophys. Res., 105, p. 27251 | ||
| 504 | |a Yurchyshyn, V., Liu, C., Abramenko, V., Krall, J., (2006) Solar Phys., 239, p. 317 | ||
| 504 | |a Zarro, D.M., Sterling, A.C., Thompson, B.J., Hudson, H.S., Nitta, N., (1999) Astrophys. J., 520, p. 139 | ||
| 504 | |a Zhang, J., Ma, J., Wang, H., (2006) Astrophys. J., 649, p. 464 | ||
| 504 | |a Zhukov, A.N., Auchère, F., (2004) Astron. Astrophys., 427, p. 705 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a It is generally accepted that transient coronal holes (TCHs, dimmings) correspond to the magnetic footpoints of CMEs that remain rooted in the Sun as the CME expands out into the interplanetary space. However, the observation that the average intensity of the 12 May 1997 dimmings recover to their pre-eruption intensity in SOHO/EIT data within 48 hours, whilst suprathermal unidirectional electron heat fluxes are observed at 1 AU in the related ICME more than 70 hours after the eruption, leads us to question why and how the dimmings disappear whilst the magnetic connectivity is maintained. We also examine two other CME-related dimming events: 13 May 2005 and 6 July 2006. We study the morphology of the dimmings and how they recover. We find that, far from exhibiting a uniform intensity, dimmings observed in SOHO/EIT data have a deep central core and a more shallow extended dimming area. The dimmings recover not only by shrinking of their outer boundaries but also by internal brightenings. We quantitatively demonstrate that the model developed by Fisk and Schwadron (Astrophys. J. 560, 425, 2001) of interchange reconnections between "open" magnetic field and small coronal loops is a strong candidate for the mechanism facilitating the recovery of the dimmings. This process disperses the concentration of ∈"open" magnetic field (forming the dimming) out into the surrounding quiet Sun, thus recovering the intensity of the dimmings whilst still maintaining the magnetic connectivity to the Sun. © 2008 Springer Science+Business Media B.V. |l eng | |
| 536 | |a Detalles de la financiación: National Aeronautics and Space Administration | ||
| 536 | |a Detalles de la financiación: Belgian Federal Science Policy Office | ||
| 536 | |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas, 20326 | ||
| 536 | |a Detalles de la financiación: Centre National de la Recherche Scientifique | ||
| 536 | |a Detalles de la financiación: Acknowledgements We sincerely thank the anonymous referee for helpful comments, which improved the clarity and readability of this work. G.D.R.A and K.S. are grateful to STFC for support. L.v.D.G. acknowledges Hungarian government grant OTKA T048961. P.D. and C.H.M. acknowledge financial support from CNRS (France) and CONICET (Argentina) through their cooperative science programme (N. 20326). A.N.Z. acknowledges support from the Belgian Federal Science Policy Office through the ESA-PRODEX programme. J.L. was supported by NASA and CISM, an NSF Science and Technology Center. | ||
| 593 | |a Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom | ||
| 593 | |a Observatoire de Paris, LESIA, UMR 8109 (CNRS), Meudon Principal Cedex 92195, France | ||
| 593 | |a Konkoly Observatory of the Hungarian Academy of Sciences, Budapest, Hungary | ||
| 593 | |a Solar-Terrestrial Center of Excellence - SIDC, Royal Observatory of Belgium, Avenue Circulaire 3, Brussels 1180, Belgium | ||
| 593 | |a Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow 119992, Russian Federation | ||
| 593 | |a Instituto de Astronomía Y Física del Espacio, CONICET-UBA, CC. 67, Suc. 28, Buenos Aires 1428, Argentina | ||
| 593 | |a Science Applications International Corporation, 10260 Campus Point Drive, San Diego, CA 92121, United States | ||
| 690 | 1 | 0 | |a CORONA |
| 690 | 1 | 0 | |a CORONAL MASS EJECTIONS |
| 690 | 1 | 0 | |a LOW CORONAL SIGNATURES |
| 690 | 1 | 0 | |a MAGNETIC FIELDS |
| 690 | 1 | 0 | |a QUIET SUN |
| 700 | 1 | |a Van Driel-Gesztelyi, L. | |
| 700 | 1 | |a Démoulin, Pascal | |
| 700 | 1 | |a Zhukov, A.N. | |
| 700 | 1 | |a Steed, K. | |
| 700 | 1 | |a Harra, L.K. | |
| 700 | 1 | |a Mandrini, Cristina Hemilse | |
| 700 | 1 | |a Linker, J. | |
| 773 | 0 | |d 2008 |g v. 252 |h pp. 349-372 |k n. 2 |p Sol. Phys. |x 00380938 |w (AR-BaUEN)CENRE-2238 |t Solar Physics | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-55349118465&doi=10.1007%2fs11207-008-9255-z&partnerID=40&md5=7e8cfc3fd3df17834294905848a65e3b |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1007/s11207-008-9255-z |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00380938_v252_n2_p349_Attrill |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v252_n2_p349_Attrill |y Registro en la Biblioteca Digital |
| 961 | |a paper_00380938_v252_n2_p349_Attrill |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 83246 | ||