NBYM04 Introduction 1.“Symposium on Nobeyama Radioheliograph” –1990 November NRO 2.“Kofu symposium – New look at the Sun with emphasis on advanced.

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Presentation transcript:

NBYM04 Introduction 1.“Symposium on Nobeyama Radioheliograph” –1990 November NRO 2.“Kofu symposium – New look at the Sun with emphasis on advanced Observations of coronal dynamics and flares” –1994 September Kofu 3.“Solar physics with radio observations” –1998 October 27 – Kiyosato 4.“Solar physics with the Nobeyama Radioheliograph” － 2004 October 26 – Kiyosato

Nobeyama Radioheliograph Proposal: early 1980s (Prof. Haruo Tanaka, 1985) Reorganization: NAOJ (1988) Merger of Toyokawa and Nobeyama groups Construction: 1990 – 1991 (Prof. Keizo Kai, 1991) –YOHKOH launched 1991 August Routine observation 1992 June/July Dual frequency 1995 Another reorganization NSRO/NAO/NINS(2004)

Main target Particle acceleration mechanisms in solar flares? –No answer yet Existing MHD solar flare theory does not include particle acceleration Observed features do not fit to the existing theory –Two- or multi-loop configuration –Non-thermal loop (no evaporation from footpoints) –Flare associated oscillations

Flare geometry found by NoRH

Nonthermal electron injection (filling process of nonthermal loop with light speed) Earth size

Non-thermal and thermal loop

Standard flare model/scenario

Other subjects Eruptions –Uniform coverage for a long time (weather, good maintenance, one solar cycle), continuum emission, and high cadence Active regions –Umbral oscillation (solar cycle dependence) –Magnetic field measurements Quiet sun –Polar brightening, dark filaments/prominences (solar cycle dependence)

Proposal of a new solar flare scenario NoRH event on 1993 January 2 moviemovie Two (multiple) loop configuration, non-thermal loop Ballooning/Flute instability (interchange instability) –Finite(high) beta plasma in a curved magnetic field –Thermal(confined) / flow plasma energy is the energy source for solar flares –Turbulence (power law energy distribution and power law distribution of power spectra of microwave light curves.)

Power law energy distribution log (E) log (N) N(E)dE = A E -δ dE

A new flare model/scenario Plasma/particle Ballooning instability (interchange instability) Plasma turbulence

International user group Open data policy INTERNET development All the data since the beginning are online Event lists, event images (Yokoyama) Ejection lists, images (Shimojo) NoRH software/SSW and analysis manuals (Yokoyama et al.) Data analysis opportunities (CDAW like) Invitation of international users to Nobeyama

Publications Refereed journals: 120 papers Proceedings: 194 papers More publications in refereed journals

Proceedings of this symposium Electronic files on CD-ROM Proceedings book (review reports) Special issue for NoRH: Publication of Astronomical Society of Japan (original contributions+one invited review paper) We encourage you to submit original papers including NoRH data to PASJ special issue.