1964
DOI: 10.1016/0032-0633(64)90034-0
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Problems of differentiation of flares with respect to geophysical effects

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Cited by 28 publications
(18 citation statements)
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“…Such an investigation is also of interest for the study of solar magnetic fields. Indeed, recent observations (Frank and Gurnett, 1972;Alvarez et al, 1972;Linet al, 1973) have clearly shown that type III bursts are excited by fast electrons, in full agreement with the plasma hypothesis initiated by Wild et al (1959). These particles are escaping through the corona and the interplanetary medium on a scatter free mode.…”
Section: Introductionsupporting
confidence: 68%
“…Such an investigation is also of interest for the study of solar magnetic fields. Indeed, recent observations (Frank and Gurnett, 1972;Alvarez et al, 1972;Linet al, 1973) have clearly shown that type III bursts are excited by fast electrons, in full agreement with the plasma hypothesis initiated by Wild et al (1959). These particles are escaping through the corona and the interplanetary medium on a scatter free mode.…”
Section: Introductionsupporting
confidence: 68%
“…The type of SID for which worldwide coverage has been most nearly complete in recent years is the Short-Wave Fade (SWF). We therefore have studied the occurrence of SWF's with the 69 flares of importance N2 in regions with small or no spots, 1956-1969, and have compared the results with similar information for all flares of importance ~2 observed during the IGY (1957IGY ( .5-1958 (Dodson and Hedeman, 1964). A summary of this comparison is shown in Table III.…”
Section: Ionizing Radiationmentioning
confidence: 99%
“…Approximately 80?/0 of the flares of importance )2 were accompanied by X-ray enhancement (2-12 A) at least as great as 4 times the ambient quiet Sun, whether or not they were located in regions with significant spots. For X-ray bursts of greater intensity, flares in spotted Dodson and Hedeman (1964).…”
Section: Ionizing Radiationmentioning
confidence: 99%
“…http://www.livingreviews.org/lrsp-2012-3 3.8 "Problem" and "stealth" CMEs So-called "problem" geomagnetic storms lack historically obvious signatures of related solar activity, such as flares and large disappearing filaments (e.g., Dodson and Hedeman, 1964;McAllister et al, 1996, and references therein). An event on 6 -10 January 1997 was the first such problem storm for which the antecedent CME was actually observed (Webb et al, 2000b).…”
Section: Living Reviews In Solar Physicsmentioning
confidence: 99%