ϊA@@@@@@@@@@@@@@@@@Contents
Contents
Enome, S. and Hirayama, Tccccccccccccccccccccccccc..ϊ@
Contents@ccccccccccccccccccccccccccccccccccccϊA
Program@ccccccccccccccccccccccccccccccccccccϊH
Yohkoh
Reviews:
Thermal Plasmas in the Solar Corona: the Yohkoh Soft X-Ray Observations
High-energy Solar Flare Observations by Yohkoh: A Review
Kosugi,Tcccccccccccccccccccccccccccccccccc.11
The
Nobeyama Radioheliograph Introductions:
The Nobeyama Radioheliograph - Hardware System -
Nishio, M., Nakajima, H., Enome, S., Shibasaki, K., Takano, T., Hanaoka,
Y., Torii, C., Shiomi, Y., Sekiguchi, H., Bushimata, T., Kawashima, S.,
Shinohara, N., Koshiishi, H., Kosugi, T., Sawa, M., Kai, K., Irimajiri, Y.,
Nohmi, H., Honda, K., Shinohara, H., Ito, T., Miyawaki, M., Imoto, A.,
Takabayashi, T., Nishikawa, K., Futagawa, N., Tanaka, S., Morikawa, H.,
Kitahara, Y., Harakawa, K., and Mishima, Kccccccccccccccccc. 19
Processing of the Nobeyama Radioheliograph Data
Hanaoka, Y., Shibasaki, K., Nishio, M., Enome, S., Nakajima, H., Takano,
T., Torii, C., Sekiguchi, H., Bushimata, T., Kawashima, S., Shinohara, N.,
Irimajiri, Y., Koshiishi, H., Kosugi, T., Shiomi, Y., Sawa, M., and Kai.K....................35
The Nobeyama Radioheliograph Data use
Shibasaki, K., Enome, S., Nakajima, H., Nishio, M., Takano,T., Hanaoka,
Y., Torii, C., Sekiguchi, H., Kawashima, S., Bushimata, T., Shinohara, N.,
Koshiishi, H., and Shiomi, Yccccccccccccccccccccccccc45
I.
Coronal Dynamics and Quiet
Observations of the structure and dynamics of coronal loops.
Strong, K. Tcccccccccccccccccccccccccccccccc..53
The X-ray intensity distribution of the solar corona and its variability.
Hara, H. cccccccccccccccccccccccccccccccccc57
Active-region transient brightenings and the heating of active region corona
Microflaring at the feet of large active region loops.
Porter, J.,
P. A., and
Observzational signatures of nanoflare heating
Poletto, G. and Kopp, Rccccccccccccccccccccccccccc 71
Contents@@@@@@@@@@@@@@@@@@@ ϊB
Shibata, K., Yokoyama, T., and Shimojo, Mcccccccccccc.cccccc.75
Observation of 17GHz radio emission from X-ray bright points.
kundu, M. R., Shibasaki, K., Enome, S., and Nitta, Nccccccccccccc.. .79
Ejection
of heated mass into a helix-like structure from active region NOAA 7172 on
Uchida Y., Fludra, A., Khan, J., and McAllister, Accccccccccccccc 83
Observations of enhanced coronal heating in sheared magnetic fields.
P.A., and
Dynamic coronal heating by magnetic flux interaction.
Priest,E.Rccccccccccccccccccccccccccccccccc..93
Characteristics
of microflares seen in helium-like sulphur spectra: GOES A-class flares
during the minimum activity phase.
Watanabe, Teccccccccccccccccccccccccccccccc.. .99
Low-speed solar winds observed at
distances of@20-60 Rs
and coronal structure@of
Kojima, M., Misawa, H., Kozuka, Y., Yamauchi, Y., Watanabe, H., and
Manoharan, P. Kcccccccccccccccccccccccccccccc105
Real time prediction and observation of interplanetary events.
Manoharan, P. K., Ananthakrishnan, S., Detman, T. R., Dryer, M., Lein-
bach, H., Kojima, M., Watanabe, Ta., and Khan, Jccccccccccccccc109
Spectroscopic observations of
coronal emission lines and their relation to soft X-ray
Ichimoto, K., Kumagai, K., Sakurai, T., Hara, H., Takeda, A., and Yohkoh
SXT Teamccccccccccccccccccccccccccccccccc.113
U.Flares
Energy transport mechanisms and the event of 16th December 1991.
Culhane, J. L., Phillips, A. T.,
Kosugi, T., Inda-Koide, M., and Pike, C. D. ccc...117
Positron annihilation line from
the 15 November 1991 Flare.
Kawabata,
K., Yoshimori, M., Suga, K., Morimoto, K., Hiraoka, T., Sato, J.,
and Ohki, Kcccccccccccccccccccccccccccccccc123
Hard and soft X-ray observations
of a super-hot thermal flare of 6 February, 1992.
Kosugi, T., Sakao, T., and Masuda, S.,
Hara, H.,
H.Scccccccccccccccccccccccccccccccccccc127
Yohkoh Bragg Crystal Spectrometer (BCS)
observations of the 6-Feb-1992 Limb
A very small two-ribbon flare of GOES X-ray
class B6.7.
Suematsu Y. cccccccccccccccccccccccccccccccc135
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Temperature
analysis of the post-flare loops of June 25-26, 1992.
Anwar, B., Hiei, E., Hudson, H. S., Acton, L. W., Lemen, J. R., and Metcalf,
T.Rccccccccccccccccccccccccccccccccc..cc 137
Alignment
of radio, soft X-ray and hard X-ray images of sources in impulsive
and gradual phases of the flare of 1992 August 17-18.
Enome, S., Nakajima, H., Shibasaki, K., Nishio, M., Takano, T., Hanaoka,
Y., Torii, C., Shiomi, Y., Sekiguchi, H., Bushimata, T., Kawashima, S.,
Shinohara, N., Irimajiri, Y., Koshiishi, H., Choi, Y. -S.,
M., Takakura, T., Sakao, T.,and Kosugi, T. ................................................................141
A comparison of hard X-ray, soft X-ray and microwave sources in solar flares.
Yaji, K., Kosugi, T., Sakao, T., Masuda, S., Inda-Koide, M. and Hanaoka, Y. cc..143
Kitai R., Kurokawa, H., Funakoshi, Y., Nakai, Y., Shibata, K., Yaji, K.,
Nitta, N .,and Yohkoh Team and NAOJ Flare Telescope Team ......cccc.......... 147
Evolution and radio activity of a flare productive active region NOAA 7321.
Nishio, M., Takakura, T., Ikeda, H., Nakajima, H., Enome, S., Shibasaki, K.,
Takano, T., Hanaoka, Y., Choi, Y.-S., and Koshiishi, H ........................................... 151
Evolution of flare source
inferred from hard X-ray and radio observation: Solar burst
Takakura, T., and HXT Group: Nishio, M., and the Radioheliograph Groupcc. 157
Yohkoh
HXT/SXT observations of a two-loop interaction solar flare on 9 December
Inda-Koide, M. ................................. cccccccccccccccccccc161
OVRO and NRO observations of the solar flare on 1993 June 3.
Gary, D., Enome, S., and Bruner, M. ........................................................................ 165
Hard X-ray imaging observations of footpoint sources in impulsive solar flares.
Sakao, T., Kosugi, T., Masuda, S., Yaji, K., Inda-Koide, M., and
Makishima, K ............................................................................................................
169
The electron density in the localized bright regions at the tops of flare loops.
Doschek, G. A.. ...........................................................................................................173
Morphology of the 10 million degree plasma in solar flares and the failure of the
chromospheric evaporation model.
Seely, J. F.,
Feldman, U.,
Doschek,G.
A., Strong, K.
T.,
Uchida, Y., and Tsuneta, S. ....................................................................................... 177
Long duration events observed with the Nobeyama Radioheliograph.
Hanaoka,Y. ................................................................................................................. 181
Morphological development of gradual nonthermal microwave flares.
Nakajima, H., Enome, S., Shibasaki, K., Nishio, M., Takano, T., Hanaoka,
Y., Torii, C., Shiomi, Y., Sekiguchi, H., Bushimata, T., Kawashima, S.,
Shinohara, N., and Koshiishi, H. .............................................................................. 185
BCS spectra from flares on 6th September 1992.
Kato, T., and Fujiwara, T., BCS Group ..................... ccccccccccccc..191
HΏ and X-ray signatures of chromospheric heating observed in solar flares.
Wülser, J.-P., Canfield, R. C., Sakao, T., Masuda, S., Kosugi, T., and
Tsuneta, S. .................................................................................................................. 195
Contents@@@@@@@@@@@@@@@@@ @ϊD
Energy transport during a solar
flare: VLA observations of the
M1.9 flare of 20 Aug.
Bastian, T. S., Nitta, N., Kiplinger, A. L., and Dulk, G. A. c...............................199
Multiwavelength observations of a solar flare.
White, S. M., Silva, A. S., Pater, I. de, Lin, R. P., Gary, D. E., Hudson, H.
S., Doyle, J. G., Hagyard, M. J., and Kundu, M. Rccccccccc.............. c203
Structural changes of radio sources during early phase of small bursts.
Shibasaki, K., Enome, S., Nakajima, H., Nishio, M., Takano, T., Hanaoka,
Y., Torii, C.,
Sekiguchi, H., Kawashima, S., Bushimata, T.,
Shinohara, N.,
Koshiishi, H., and Shiomi, Y. ....................................................................................... 205
Vertical structure of hard X-ray sources in solar flares.
Masuda, S..................................................................................................................209
Thermal and nonthermal energizations
in solar flares: Soft X-ray spectroscopic and
Cheng, C.-C., Rilee, M., and Uchida, Y......................................................................... 213
Evidence for both electron acceleration and direct heating in solar flares.
Dennis, B. R., Holman, G. D., Hudson, H. S., Kosugi, T., Strong, K. T., and
Zarro, D. ........................................................................................................................ 217
Studying solar flares with Yohkoh and the Compton Gamma-Ray Observatory.
Zarro, D.M., Mariska, J. T., and Dennis, B. Rccc.................................................. 221
DC electric fields in solar flares: Theory meets observation.
Benka,
S.........................................................................................................................225
Stochastic
acceleration in the diffusion region and the
structure of slow shocks in
Hirayama, T.. ................................................................................................................231
The current profile and energy release in
solar flares.
Impulsive acceleration and bulk heating of flare plasma by plasma turbulence.
Petrosian, V. ............................................................................................. 239
Experimental
investigation of three dimensional magnetic reconnection by use of two
Ono, Y., Akao, T., Morita, A., Katsurai, M., and Yamada, M. ............................. 243
Computer simulations on the fast reconnection mechanism.
Ugai, M. ....................................................................................................................... 247
Particle dynamics in two colliding plasmas.
Takeuchi, S. ..................................................................................................................251
Coalescence of two current loops
with a kink instability simulated by a 3-D
EM
Nishikawa, K.,
Evolution of coronal mm-wave sources.
Krüger, A., Hildebrandt, J., Urpo, S., and Pohjolainen, S.........................................
259
Energetic electrons and magnetic field structures in the corona.
Pick, M., Raoult, A., Trottet, G., Vilmer, N., Strong, K.,
and Magalhaes, Accc 263
ϊE@@@@@@@@@@@@@@@@@@Contents
Solar neutron events of June 4th and 6th, 1991.
Muraki,
Y., Sakakibara, S., Shibata, S.,
Murakami, K., Takahashi, K., Pyle,
K. R.,
Properties of energetic particles studied from Gamma-ray observations.
Yoshimori, M., Suga, K., Morimoto, K., Hiraoka, T., Sato, J., Kawabata, K.,
and Ohki, K. ...............................................................................................................
271
On the origin of long lasting gamma ray emission from solar flares.
Ramaty, R.and Mandzhavidze, N.............................................................................. 275
Ionization states of solar-flare particles.
Sakurai, K...................................................................................................................
279
V.Active Regions
A morphological
study of magnetic shear development in a flare-productive region
Kurokawa, H.,Kitai, R., Kawai, G., Shibata, K., Yaji, K., Ichimoto, K.,
Nitta, N., and Zhang, H.............................................................................................
283
HRTS observations of explosive
events in a flaring active region.
Dere,
K. P. and Martin, S. F.......................................................................................
289
Combined HRTS-8 sounding rocket
observations and Yohkoh soft X-ray observations
of NOAA active region 7260 at the solar limb.
Korendyke, C. M., Dere, K. P., Brueckner, G. E., Waljeski, K., and Lemen,
J.R. ...............................................................................................................................293
Evolution of active regions leading to flares.
Schmieder, B., Demoulin, P., Henoux, J.-C., Driel-Gesztelyi, L. v., Mandrini,
C., and Rovira, M. ........................................................................................................297
The photospheric-to-coronal iron
abundance from X-ray lines observed by Yohkoh
Phillips,
K. J. H., Pike,C. D., Lang, J., Watanabe, Te., and Zarro, D.
M. cccc...301
Implications of coronal abundance variations.
W.Instrumentation
First CCD observations of a flare in H-epsilon and Ca-II(H).
Rolli, E......................................................................................................................... 309
The High Energy Solar Physics Mission (HESP)
Dennis B.R. ................................................................................................................
313
X. Posters
Coronal structures observed in X-rays (NIXT) and H-Ώ surges.
Schmieder,
B., Mouradian, Z., Golub, L., and Antiochos, S.. ccccccc.......... 317
Propagation
of radio waves in the sun's corona: Angular broadening in the limit of
Bastian, T. S. ................................................................................................................321
Contents@@@@@@@@@@@@@@@@@ @ϊF
The new solar submillimeter-wave telescope project (SST).
Kaufmann, P., Parada, N. J., Magun, A., Rovira, M., Ghielmetti, H., and
Levato, H....................................................................................................................... 323
Determining point spread function of space observations using bid algorithm.
Karovska, M. and Hudson, H. S. ......................................................................
327
The fine scale structure of the solar limb in a coronal hole.
Karovska, M. and Arndt, M. B..................................................................................331
Thermal
conduction in the transition
region and its effects on the energy balance of
Hammer,
R. ..................................................................................................................
335
Microflares and their related events.
Schmieder, B., Fontenla, J.,
Tandberg-Hanssen, E., and Simnett, G. M. ..................
339
Metric Type III bursts from flaring X-ray
bright points.
Kundu, M. R., Strong, K. T., Pick,
M., Harvey, K. T., Kane, S. R., White,
S.
M., and Hudson, H. S...............................................................................................
343
Study of active region magnetic
field structures using VLA radio, Yohkoh X-ray and
Gopalswamy, N., Schmahl, E. J.,
Kundu, M. R., Lemen, J. R., Strong, K.
T., Canfield, R. C., and
Beaujardiere, J. de la............................................................
347
Evolution of an active region and flare productivity.
Kundu, M. R., Shibasaki, K., Enome, S., Nitta, N., Bruner, M., Sakao, T.,
and Kosugi, T. .............................................................................................353
VLA stereoscopy of
solar active regions.
Aschwanden, M. J. and Bastian, T. Scccccccccccccccccccc...357
Rotation rates of soft X-ray coronal structures.
Kozuka, Y., Watanabe, Ta., Kojima,
M., Ohyama, M., and Saito, T. ....................... 359
A potential field model for open field lines in the active region corona.
Sakurai,
T. ...................................................................................................................
363
Numerical
simulation of reconnection between emerging flux and coronal field.
Yokoyama,
T. and Shibata, K.........................................................................................
367
The high energy gamma-ray flare of
June 15, 1991: Some evidence of prolonged
particle acceleration at the post-eruptive phase.
Akimov, V.
V., Belov, A. V., Chertok,
Magun, A., and Melnikov, V.
F.....................................................................................
371
A Search for
"Black-Light Flares"
Driel-Gesztelyi,
L. v.,
A
relation of variabilities between
the solar dust ring and the solar magnetic field.
Isobe, S.and Kumar, A. S.
...........................................................................................
379
Thermal and density structure of
the inner corona observed at the 1991 total solar
Takeda, A., Kurokawa, H., Kitai, R., and Ishiura, K. .............................................. 381
Flares in active region NOAA 7260-Role of emerging flux.
Nitta, N., Driel-Gesztelyi, L. v., Leka, K. D., Mickey, D. L., Metcalf,
T. R.,
Wülser, J.-P., Ichimoto, K.,
Sakurai, T., and Shibata, K........................................... 385
ϊG@@@@@@@@@@@@@@@@Contents
Multi spacecraft observations
and thick-target electron beam models for the 15-NOV-
McTiernan, J. M., Kane, S. R., Hurley,
K., Laros, J. G., Fenimore, E. E.,
Klebsadel,
R. W., Sommer, M., and Yoshimori, M. ....................................................
389
Long duration events in magnetic
arcades and large loops.
Fludra,
A., Jakimiec, J.,
Tomczak, M., Culhane, J. L, and
Analysis of three Yohkoh
white-light flares.
Solar wind velocity near the sun: Results from interplanetary
scintillation observa-
Tokumaru, M., Mori, H., Tanaka,
T., Kondo, T., and Yamauchi, Y. ...........................401
Evidence of additional
production of high energy neutrons during the solar flare on
Struminsky, A., Matsuoka, M., and
Takahashi, K. ..........................................
405
Red asymmetries of optical lines at the impulsive phase of solar flares.
Shoji, M. and Kurokawa, H. .......................................................................................
409
Preliminary reduction of data obtained with a full disk magnetograph.
Liu, Y., Song, G., Wang, Jingshan, and Wang, Jingxiu .....................................
413
Soft X-ray feature in active
regions associated with meter wavelength solar radio
Watari, S., Isobe, T., and Yohkoh SXT Team ....................................................417
Correlation between solar microwave bursts and hard X-ray flares.
Fu, Q., Liu, Y., and Li, C. .............................................................................................
421
List of participants ................................................................................................................425
Author index.......................................................................................................................... 435