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originally posted by: choos
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you labelled the 10^-7 correct, but you labelled the dotted lines incorrectly it should be:
20^-7, 30^-7, 40^-7... 90^-7 then 100^-7 or 10^-6
so in other words that brown line should be x0^-7, orange as x0^-6 and blue x0^-5 etc.
originally posted by: Arbitrageur
The peak of 5x10^-5 W/m^2 falls between 10^-5 and 10^-4 W/m^2 which is what makes it an M class, so that's definitely not 5x10^-4 W/m^2 as EU is saying.
You have contradicted yourself with that statement because that means more precisely 1x10^-5 and 1x10^-4 w/m^2 and since 5x10^-4 w/m^2 is outside of that range, it's not an M-class flare, in fact it has 5 times the peak energy of the most powerful M-class flare which would only have 1x10^-4 W/m^2.
originally posted by: ElectricUniverse
Look, it's not my problem anymore if you don't want to admit you made a mistake. Yes, an M5 flare tells you the overall energy of the flare, but the plotted data shows you where it falls. M5 falls between a 10^-5 and 10^-4 w/m^2.
No the bottom if the M-class flare category would be 1 x 10^-5 W/m^2. The top is 1x10^-4 W/m^2. 5 x 10^-5 W/m^2 is in between those two so it's sort of in the middle of the M-class range though on a logarithmic scale like the graph we've been looking at, 5 looks closer to the top end of the range and not exactly in the middle.
If it was an M5 with 10^-5 w/m^2 like you claim it is, it would fall EXACTLY on the bottom of the M flare class
Again you've contradicted yourself here. That is 5 times more powerful than the top of the range you just provided when you said " M5 falls between a 10^-5 and 10^-4 w/m^2. " 5x10^-4 w/m^2 is NOT between a 10^-5 and 10^-4 w/m^2, I don't know how you can not understand this, but I guess you're not good with numbers or math, not that you should need to be to understand such a simple concept. And again 5x10-4 W/m^2 falls clearly into the X-class of the table I posted, it wouldn't be an M-class flare.
It is almost going to the top, which makes it an 0.0005 w/m^2 or an M5 10^4 w/m^2.
originally posted by: ElectricUniverse
I did not label the "dotted lines incorrectly"...
That's definitely better than ElectricUniverse's labeling, but 10^-5 is actually a single value on the graph and it was already labeled. If you want to label a range which is apparently what you're trying to do then a lower and upper limit is needed of the range, so you could label the ranges like this:
originally posted by: choos
here fixed the labelling for you:
Finally!
originally posted by: ElectricUniverse
You were right about that flare being 10^-5 w/m^2.
Technically I didn't exactly say that "cosmic rays cannot affect the climate". What I said was increasing soft X-rays from 5x10^-7 W/m^2 to 100 times that or even 1000 times that to 5x10^-4 W/m^2 is a measurable but not a significant amount compared to 1366 W/m^2, do you disagree with that?
But you are wrong in your claims that cosmic rays cannot affect the climate. You are also ignoring the fact that the Sun's visible light has been increasing and has been warming Earth's Troposphere which is something that was not expected.
Cosmic Dust, Refraction and Emissivity
Frank H. Makinson*
Abstract—Cosmic dust is pervasive within our galaxy and it is reasonable to suspect it is dispersed in various ways
throughout the universe. Cosmic dust has emissivity when exposed to electromagnetic energy sources. The emissivity of cosmic dust contributes to cosmic radio noise and concentrations of it alters electromagnetic waves by refraction. Cosmic dust is concentrated in our Sun’s heliosphere and the resultant emissivity products in the micro-wave and infrared should be detectable by land based and satellite radio telescope instruments. It is possible that many of the claimed microwave and infrared measurements of the universe have in part or their entirety mapped the energy patterns of the cosmic dust in the heliosphere rather than energy patterns beyond it.
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"By analyzing both sets of data together, we could get a more definitive picture of what's going on than we could with either dataset alone," said Charles Lawrence, the U.S. project scientist for Planck at NASA's Jet Propulsion Laboratory, Pasadena, California. "The joint analysis shows that much of the signal detected by BICEP2/Keck is coming from dust in the Milky Way, but we cannot rule out a gravitational wave signal at a low level. This is a good example of how progress is made in science, one step at a time."
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NEW OBSERVATIONS OF THE SOLAR 0.5 – 5 KEV SOFT X-RAY SPECTRUM
AMIR CASPI1,3, THOMAS N. WOODS1, and HARRY P. WARREN2
1 Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA
2 Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
Received 2014 October 28; accepted 2015 January 23; published 2015 March 18
ABSTRACT
The solar corona is orders of magnitude hotter than the underlying photosphere, but how the corona attains such
high temperatures is still not understood. Soft X-ray (SXR) emission provides important diagnostics for thermal processes in the high-temperature corona, and is also an important driver of ionospheric dynamics at Earth. There is a crucial observational gap between ∼0.2 and ∼4 keV, outside the ranges of existing spectrometers. We present observations from a new SXR spectrometer, the Amptek X123-SDD, which measured the spatially integrated solar spectral irradiance from ∼0.5 to ∼5 keV, with ∼0.15 keV FWHM resolution, during sounding rocket flights on 2012 June 23 and 2013 October 21. These measurements show that the highly variable SXR emission is orders of magnitude greater than that during the deep minimum of 2009, even with only weak activity. The observed spectra show significant high-temperature(5–10 MK) emission and are well fit by simple power-law temperature distributions with indices of ∼6, close to the predictions of nano flare models of coronal heating. Observations during the more active 2013 flight indicate an enrichment of low first-ionization potential elements of only ∼1.6, below the usually observed value of ∼4, suggesting that abundance variations may be related to coronal heating processes. The XUV Photometer System Level 4 data product, a spectral irradiance model derived from integrated broadband measurements, significantly overestimates the spectra from both flights, suggesting a need for revision of its non-flare reference spectra, with important implications for studies of Earth ionospheric dynamics driven by solar SXRs.
Key words:plasmas–radiation mechanisms: thermal–Sun: corona–Sun: X-rays, gamma-rays
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