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I: “The Magnetic and Velocity Fields of Solar Active Regions”, IAU Colloq. 141 (Ref. I), Zirin, H, Ai, G, and Wang, H (eds.), APS Conf. Series (San Francisco), 46, 1993Google Scholar
Acton, D and Smithson, R: 1992, Appl. Opt.31, 3161Google Scholar
Dunn, R and Smartt, R: 1991, Adv. Space Res.11, No. 5, 139Google Scholar
Dunn, R, Streander, G, Hull, E, and Wilkins, L: 1991, SPIE Conf. “Active and Adaptive Opt. Syst.”, 88Google Scholar
Fang, C: 1993, in Sakurai, T (ed), “Proc Japan-China Workshop on Solar Phys.”Google Scholar
Hammerschlag, R, and Zwaan, C: 1992, Ann. Rep. of the Sterrekundig Inst.UtrechtGoogle Scholar
Ichimoto, K, Sakurai, T, Nishino, Y, Shinoda, K, Kumagai, Noguchi M, Imai H, K, Irie, M, Miyashita, M, Tanaka, N, Sano, I, Suematsu, Y, and Hiei, E: 1993, Ref. I, p. 166Google Scholar
Jones, H, Duvall, T, Harvey, J, Mahaffey, C, Schwitters, J, and Simmons, J: 1992, Solar Phys.139, 211Google Scholar
Keller, C, Aebersold, F, Egger, U, Povel, H, Steiner, P and Stenflo, J: LEST Tech. Rep. No. 53Google Scholar
von der Lühe, O: 1991, Adv. Space Res.11, No.5, 275Google Scholar
Wang, H, Varsik, J, Zirin, H, Canfield, R, Leka, K, and Wang, J: 1992, Solar Phys.142, 11Google Scholar
Zhang, B, Deng, Y, and Li, Y: 1993, in Sakurai, T (ed), “Proc Japan-China Workshop on Solar Phys.”Google Scholar
I:
I: “The Magnetic and Velocity Fields of Solar Active Regions”, IAU Colloq. 141 (Ref. I), Zirin, H, Ai, G, and Wang, H (eds.), APS Conf. Series (San Francisco), 46, 1993Google Scholar
Alissandrakis, CE, Lubyshev, BI, Smolkov, GYa, Krissinel, BB, Treshkov, TA, Miller, VG, and Kardapolova, NN: 1992, Solar Phys.142, 341Google Scholar
Alissandrakis, CE, Gelfreikh, GB, Borovik, VN, Korzhavin, AN, Bogod, VM, Nindos, A, and Kundu, MR: 1993, Astron. Astrophys. 270, 509Google Scholar
Bogod, VM, Vatrushin, SM, Abramov-Maximov, VE, Tsvetkov, SV, and Dikij, VN: 1993, Ref. I, p. 306Google Scholar
Costa, JER, Correia, E, Kaufmann, P, Herrmann, R, and Magun, A: 1992, Ref. I, p. 177Google Scholar
Enome, S: 1992, in “Eruptive Solar Flares”, Svestka, Z, Jackson, BV, and Machado, ME (eds.), IAU Colloq. 133, Lecture Notes in Physics 399, Springer-Verlag (Berlin), p. 314Google Scholar
Enome, S, Nakajima, H, Shibasaki, K, Nishio, M, Takano, T, Hanaoka, Y, Torii, C, Sekiguchi, H, Kawashima, S, Bushimata, T, Shinohara, N, Irimajiri, Y, Koshiishi, H, Kosugi, T, Shiomi, Y, Sawa, M, and Kai, K: 1993, Ref. I, p 310Google Scholar
Gelfreikh, GB.Bogod, VM, Abramov-Maximov, VE, and Tsvetkov, SV: 1993, Ref. I, p. 271Google Scholar
Herrmann, R, Magun, A, Costa, JER, Correia, E, and Kaufmann, P: 1992, Solar Phys.142, 157Google Scholar
Hurford, GJ and Gary, DE: 1989, Proc. Max ‘91 Workshop #1, p. 328Google Scholar
Nakajima, H, Nishio, M, Enome, S, Shibasaki, K, Takano, T, Hanaoka, Y, Torii, C, Sekiguchi, H, Bushimata, T, Kawashima, S, Shinohara, N, Irimajiri, Y, Koshiishi, H, Kosugi, T, Sawa, M, and Kai, K: 1993, Special Issue, Proc. IEEE: “Design and Instrumentation of Antennas for Deep Space Telecommunications and Radioastronomy”Google Scholar
Stähli, , Gary, DE, and Hurford, GJ: 1990, Solar Phys. 125, 343Google Scholar
I: “The Magnetic and Velocity Fields of Active Regions”, IAU Colloq. 141, Zirin H, Ai G, and Wang H (eds.), ASP Conf. Series (San Francisco), 46, 1993.Google Scholar
II:
II: “Solar Polarimetry”, Proc. NSO/SP Summer Workshop, November, L (ed.) New Mexico, 1991.Google Scholar
III:
III: “The Solar Cycle”, Proc. NSO/SP Summer Workshop, Harvey, KL (ed.), ASP Conf. Series (San Francisco), 27, 1992.Google Scholar
IV:
IV: “Sunspots: Theory and Observations”, NATO ASI Series C: 375, Thomas, JH and Weiss, NO (eds.), Kluwer (Dordrecht), 1992.Google Scholar
V:
V: “Dynamics of Solar Flares”, Proc. Flares22 Chantilly Meeting, Schmieder, B, and Priest, ER (eds.), Meudon, 1991.Google Scholar
VI:
VI: “Eruptive Solar Flares”, IAU Colloq.133, Svestka, Z, Jackson, BV, and Machado, ME (eds.), Lect. Notes Phys. 399, Springer (Berlin), 1992.Google Scholar
VII:
VII: “The Sun and Cool Stars: Activity, Magnetism, Dynamos”, IAU Colloq.130, Tuominen, I, Moss, D, and Rüdiger, G (eds.), Lect. Notes Phys.380, Springer (Berlin), 1991.Google Scholar
VIII:
VIII: “Initial Results from Yohkoh”, Special Feature, Publ. Astron. Soc. Japan44, 1992.Google Scholar
IX:
IX: “Advances in Solar System Magnetohydrodynamics”, Priest, ER and Hood, AW (eds.), Cambridge U. Press, 1991.Google Scholar
X:
X: “Solar Interior and Atmosphere”, Cox AN, Livingston WC, and Matthews, MS (eds.), The Univ. of Arizona Press (Tucson), 1991.Google Scholar
XI:
XI: “The Sun: A Laboratory for Astrophysics”, Schmelz, JT and Brown, JT (eds.), Kluwer (Dordrecht), 1992.Google Scholar
Kosugi, T: 1993, in “Physics of Solar and Stellar Coronae”, Vaiana Memorial Symp., G. S., Linsky, JL and Serio, S (eds.), Kluwer (Dordrecht), in pressGoogle Scholar
Kurokawa, Het al.: 1992, Publ. Astron. Soc. Japan44, L129Google Scholar
Tsuneta, S and Lemen, J: 1993, in “Physics of Solar and Stellar Coronae”, Vaiana Memorial Symp., G. S., Linsky, JL and Serio, S (eds.), Kluwer (Dordrecht), in pressGoogle Scholar
Uchida, Y and Sakurai, T: 1980, in “Solar Flares”, Skylab Workshop, Sturrock, PA (ed.), U. Colorado Press, 110, p. 67Google Scholar
Leikov, N, Akimov, W, Volzhenskaya, VA, Kalinkin, LF, Nesterov, VE, Galper, AM, Zemskov, VM, Oserov, YV, et al: 1993, Astron. Astrophys., Suppl. Ser. 97, No. 1, 345Google Scholar
Mandzhavidze, N and Ramaty, R: 1992, Astrophys. J. 389, 739Google Scholar
Ramaty, R and Mandzhavidze, N: 1993, “High Energy Solar Phenomena”, AIP Conf. Proc. 294Google Scholar
Rieger, E and Marschhãuser, H: 1991, Max ‘91 Workshop #3 Proc., p. 68Google Scholar
Ryan, J, Forrest, D, Lockwood, J, Loomis, M, McConnell, M, Morris, D, Webber, W, Rank, G, et al:1993, AIP Conf. Proc. 280, 631Google Scholar
IAUC141= “The Magnetic and Velocity Fields of Solar Active Regions”, IAU Colloq. 141, Zirin, H, Ai, G, and Wang, H (eds.), Astron. Soc. PacificGoogle Scholar
Abramenko, VI, Gopasyuk, SI and Ogir, MB: 1991, Solar Phys. 134, 287Google Scholar
Aly, JJ, 1991: Astrophys. J. Lett. 375, L61Google Scholar
Canfield, RC, de, laBeaujardière, JF and Leka, KD: 1991, Phil. Trans. Royal Soc. London, 336, 381Google Scholar
Wolfson, R and Low, BC: 1992, Astrophys. J. 391, 353Google Scholar
I:
I:“Dynamics of Solar Flares”, Flares 22 Workshop, Schmieder, B & Priest, ER (eds.), Obs. de Paris, DASOP, 1991Google Scholar
II:
II:“Max ‘91/SMM Solar Rares: Observations and Theory”, 3rd Max’91 Workshop, Winglee, RM and Kiplinger, AL (eds.), Colorado, U.(Boulder), 1991Google Scholar
III:
III:“Spectral Line Formation in Plasmas Under Extreme or Unusual Conditions”, Peyraud, N, Heinzel, P & Hooper, CF (eds.), J.Quant.Spectrosc.Radiat.Transfer44, No. 1, 1990Google Scholar
IV:
IV:“Eruptive Solar Flares”, IAU Colloq. 133, Svestka, Z, Jackson, BV and Machado, ME (eds), Lect. Notes Phys.399, Springer-Verlag (Berlin), 1992Google Scholar
V:
V:“Flare Physics in Solar Activity Maximum 22”, Uchida, Y, Canfield, RC, Watanabe, T and Hiei, E (eds.), Lect. Notes Phys.387, Springer-Verlag (Berlin), 1991Google Scholar
VI:
VI:“Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition”, Proc. First SOHO Workshop, Mariska, JT, Domingo, V, and Poland, AI (eds.), ESA SP-348 (ESTEC), 1992Google Scholar
VII:
VII:“Initial Results from Yohkoh”, Special Feature, Publ. Astron. Soc. Japan44, No. 5, 1992.Google Scholar
VIII:
VIII:“Physical Processes in Solar Flares”, Somov, BV, Kluwer (Dordrecht), 1992Google Scholar
IX:
IX:“Plasma Loops in the Solar Corona”, Bray, RJ, Cram, LE, Durrant, CJ and Loughhead, RE, Cambridge Univ. Press (Cambridge), 1991Google Scholar
X:
X:Haisch, B and Strong, KT, Ann. Rev. Astron. Astrophys. 29, 275, 1991Google Scholar
XI:
XI:Zirin, H, MacKinnon, A and McKenna-Lawlor, SMP, in “Solar Interior and Atmosphere”, Cox, AN, Livingston, WC & Matthews, MS (eds.), Arizona, U.Press (Tucson), 1991Google Scholar
Aboudarham, J, Chambe, G, Feautrier, N & Hénoux, JC: 1992a, in Faurobert-Scholl, M, Frisch, H, and Mein, N, (eds.), “Méthodes de determination des champs magnétiques solaires et stellaires”, Obs. de Paris, p. 163Google Scholar
Zharkova, VV and Kobylinsky, VA: 1993, Solar Phys.143, 259Google Scholar
I
I: “Plasma Loops in the Solar Corona”, Bray, RJ, Cram, LE, Durrant, CJ, and Loughhead, RE: Cambridge University Press1991.Google Scholar
II
II: “Guide to the Sun”, Phillips, KJH: Cambridge University Press, 1992.Google Scholar
III
III: “Advances in Solar System Magnetohydrodynamics”, Priest, ER and Hood, AW (eds.): Cambridge University Press, 1991.Google Scholar
IV
IV “The Sun: A Laboratory for Astrophysics”, Schmelz, JT and Brown, JC (eds.): NATO ASI Series, Kluwer (Dordrecht) 1992.Google Scholar
V
V: “Dynamics of Solar Flares”, Schmieder, B and Priest, E. (eds.): Obs. deParis, DASOP, 1991.Google Scholar
VI
VI “Flare Physics in Solar Activity Maximum 22”, Uchida, Y, Canfield, RC, Watanabe, T and Hiei, E (eds.): Lect. Notes Phys.387, Springer (Berlin), 1991.Google Scholar
VII
VII “The Physics of Solar Flares”, Culhane, JL. and Jordan, C. (eds.): 1991, Cambridge University Press.Google Scholar
VIII
VIII “Eruptive Solar Flares”, IAU Colloq. 133, Svestka, Z, Jackson, BV, and Machado, ME (eds.), Lect. Notes Phys.399, Springer (Berlin)1992.Google Scholar
IX
IX “Fundamental Problems in Solar Activity”, Pick, M and Machado, ME (eds.), Adv. Space. Res.13, No. 9, 1993.Google Scholar