Vancanneyt Sander Posted November 7, 2022 Share Posted November 7, 2022 1 uur terug, Bry zei: Do filaments cause more pronounced short, sharp spikes in solar wind density like we’re seeing right now? That’s normal for the solar wind to be bumpy. Solar wind speed is measured by measuring the speed of solar protons on the sensor. The more protons per cm3 the more accurate the speed, the less protons less accurate. So one proton could hit at bigger speed than the other. So every minute the protons that hit are counted and the average speed, but as the number of protons defer and the speed varies it gives a more bumpy look. 2 1 Link to comment Share on other sites More sharing options...
fanaticstargazer Posted November 8, 2022 Share Posted November 8, 2022 On 10/14/2022 at 3:07 PM, Jesterface23 said: It was, errored data. The ACE satellite had short periods of missing data prior, then a big gap afterwards. The DSCOVR and SOHO satellites never had spikes around that time, but every once in a while they have their own glitches. When you look at solar wind data, you are likely looking at a mix of ACE and DSCOVR data and you may not know when it switches back and forth. On 10/14/2022 at 8:34 PM, Orneno said: Personal anecdotal feelings are not really reliable scientific evidence. absence of data neither On 10/25/2022 at 9:26 PM, SunspotRager93 said: Hi, so it seems every time you have mentioned this, it's a glitch. Why do you keep asking? I am just wondering.. read my posts and you'll understand 7. nov. 2022, 08:20 utc, 68.56p/cm³ i - again - don't think it's a glitch... Link to comment Share on other sites More sharing options...
Jesterface23 Posted November 8, 2022 Share Posted November 8, 2022 19 minutes ago, fanaticstargazer said: i - again - don't think it's a glitch... Again it is the ACE satellite. Call it errored data, a malfunction, or degrading instruments then. I've probably gone through more solar wind data than everyone else here combined. Link to comment Share on other sites More sharing options...
SunspotRager93 Posted November 8, 2022 Share Posted November 8, 2022 So, now I'm confused. Is this a glitch that's happening or what? Link to comment Share on other sites More sharing options...
Solarflaretracker200 Posted November 8, 2022 Share Posted November 8, 2022 1 minute ago, SunspotRager93 said: So, now I'm confused. Is this a glitch that's happening or what? It is a glitch. Link to comment Share on other sites More sharing options...
Jesterface23 Posted November 8, 2022 Share Posted November 8, 2022 34 minutes ago, SunspotRager93 said: So, now I'm confused. Is this a glitch that's happening or what? There have been about minute long data spikes. Getting pretty old. 1 Link to comment Share on other sites More sharing options...
Bry Posted November 10, 2022 Share Posted November 10, 2022 On 11/8/2022 at 6:05 AM, Jesterface23 said: There have been about minute long data spikes. Getting pretty old. Solar wind density looks like it had some larger spikes 4-5 times today, stunningly high again... bout as many time NK fires off missiles today lol. Any thoughts if this is a glitch or other incoming events like that M5 flare the other day? Link to comment Share on other sites More sharing options...
Jesterface23 Posted November 10, 2022 Share Posted November 10, 2022 10 minutes ago, Bry said: Solar wind density looks like it had some larger spikes 4-5 times today, stunningly high again... bout as many time NK fires off missiles today lol. Any thoughts if this is a glitch or other incoming events like that M5 flare the other day? This time is it a bit of a mix of both DSCOVR and ACE having data issues recently. The only thing to blame are the satellites themselves and because we get something close to live data the are issues are here to stay. If the data doesn't look right, it probably isn't right. The data may be processed later for use as science data. One note, the IMF for both CMEs(at least when ACE doesn't have errors) are pretty much the same. When it comes to the solar wind proton density and temperature parameters, ACE had tends to have lower values while DSCOVR has higher values. That can also make things confusing when the data feed used goes back and forth. If a CME arrives from a flare or filament the IMF Bt component and solar wind velocity, density, and temperature will all spike up at the same time. 1 1 Link to comment Share on other sites More sharing options...
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