Matches in SemOpenAlex for { <https://semopenalex.org/work/W2971692007> ?p ?o ?g. }
- W2971692007 abstract "The relative amount of high temperature plasma has been found to be a useful diagnostic to determine the frequency of coronal heating on sub-resolution structures. When the loops are infrequently heated, a broad emission measure (EM) over a wider range of temperatures is expected. A narrower EM is expected for high frequency heating where the loops are closer to equilibrium. The soft X-ray spectrum contains many spectral lines that provide high temperature diagnostics, including lines from Fe XVII-XIX. This region of the solar spectrum will be observed by the Marshall Grazing Incidence Spectrometer (MaGIXS) in 2020. In this paper, we derive the expected spectral lines intensity in MaGIXS to varying amounts of high temperature plasma to demonstrate that a simple line ratio of these provides a powerful diagnostic to determine the heating frequency. Similarly, we examine ratios of AIA channel intensities, filter ratios from a XRT, and energy bands from the FOXSI sounding rocket to determine their sensitivity to this parameter. We find that both FOXSI and MaGIXS provide good diagnostic capability for high-temperature plasma. We then compare the predicted line ratios to the output of a numerical model and confirm the MaGIXS ratios provide an excellent diagnostic for heating frequency." @default.
- W2971692007 created "2019-09-12" @default.
- W2971692007 creator A5003463585 @default.
- W2971692007 creator A5004882085 @default.
- W2971692007 creator A5013811369 @default.
- W2971692007 creator A5014541338 @default.
- W2971692007 creator A5022483961 @default.
- W2971692007 creator A5026641139 @default.
- W2971692007 creator A5039082573 @default.
- W2971692007 creator A5055145635 @default.
- W2971692007 creator A5066432088 @default.
- W2971692007 creator A5091426066 @default.
- W2971692007 date "2019-09-05" @default.
- W2971692007 modified "2023-10-16" @default.
- W2971692007 title "Solar Active Region Heating Diagnostics from High Temperature Emission using the Marshall Grazing Incidence X-ray Spectrometer (MaGIXS)" @default.
- W2971692007 cites W1678742593 @default.
- W2971692007 cites W1968470864 @default.
- W2971692007 cites W1974717249 @default.
- W2971692007 cites W1988623485 @default.
- W2971692007 cites W1989283668 @default.
- W2971692007 cites W1990497610 @default.
- W2971692007 cites W1990621926 @default.
- W2971692007 cites W1994292398 @default.
- W2971692007 cites W2000756451 @default.
- W2971692007 cites W2005213880 @default.
- W2971692007 cites W2007511942 @default.
- W2971692007 cites W2011301426 @default.
- W2971692007 cites W2013207446 @default.
- W2971692007 cites W2023968127 @default.
- W2971692007 cites W2024003459 @default.
- W2971692007 cites W2035964459 @default.
- W2971692007 cites W2039624739 @default.
- W2971692007 cites W2039802832 @default.
- W2971692007 cites W2061239690 @default.
- W2971692007 cites W2062594554 @default.
- W2971692007 cites W2065173019 @default.
- W2971692007 cites W2065751499 @default.
- W2971692007 cites W2067565872 @default.
- W2971692007 cites W2067672511 @default.
- W2971692007 cites W2071966678 @default.
- W2971692007 cites W2088312212 @default.
- W2971692007 cites W2090219368 @default.
- W2971692007 cites W2094483427 @default.
- W2971692007 cites W2122020263 @default.
- W2971692007 cites W2142234851 @default.
- W2971692007 cites W2154454170 @default.
- W2971692007 cites W2160039692 @default.
- W2971692007 cites W2162103950 @default.
- W2971692007 cites W2165096720 @default.
- W2971692007 cites W2168194491 @default.
- W2971692007 cites W2339308789 @default.
- W2971692007 cites W2461306413 @default.
- W2971692007 cites W2467870285 @default.
- W2971692007 cites W2751807326 @default.
- W2971692007 cites W2762809414 @default.
- W2971692007 cites W2888532099 @default.
- W2971692007 cites W2973183337 @default.
- W2971692007 cites W3097975374 @default.
- W2971692007 cites W3099643168 @default.
- W2971692007 cites W3099809122 @default.
- W2971692007 cites W3100928422 @default.
- W2971692007 cites W3102099826 @default.
- W2971692007 cites W3103388533 @default.
- W2971692007 cites W3103483197 @default.
- W2971692007 cites W3103561458 @default.
- W2971692007 cites W3104083247 @default.
- W2971692007 cites W3104354585 @default.
- W2971692007 cites W3104873715 @default.
- W2971692007 cites W3105021787 @default.
- W2971692007 cites W3105543121 @default.
- W2971692007 cites W3171281919 @default.
- W2971692007 hasPublicationYear "2019" @default.
- W2971692007 type Work @default.
- W2971692007 sameAs 2971692007 @default.
- W2971692007 citedByCount "0" @default.
- W2971692007 crossrefType "journal-article" @default.
- W2971692007 hasAuthorship W2971692007A5003463585 @default.
- W2971692007 hasAuthorship W2971692007A5004882085 @default.
- W2971692007 hasAuthorship W2971692007A5013811369 @default.
- W2971692007 hasAuthorship W2971692007A5014541338 @default.
- W2971692007 hasAuthorship W2971692007A5022483961 @default.
- W2971692007 hasAuthorship W2971692007A5026641139 @default.
- W2971692007 hasAuthorship W2971692007A5039082573 @default.
- W2971692007 hasAuthorship W2971692007A5055145635 @default.
- W2971692007 hasAuthorship W2971692007A5066432088 @default.
- W2971692007 hasAuthorship W2971692007A5091426066 @default.
- W2971692007 hasBestOaLocation W29716920071 @default.
- W2971692007 hasConcept C120665830 @default.
- W2971692007 hasConcept C121332964 @default.
- W2971692007 hasConcept C124967146 @default.
- W2971692007 hasConcept C1276947 @default.
- W2971692007 hasConcept C159985019 @default.
- W2971692007 hasConcept C184779094 @default.
- W2971692007 hasConcept C185544564 @default.
- W2971692007 hasConcept C192562407 @default.
- W2971692007 hasConcept C198352243 @default.
- W2971692007 hasConcept C204323151 @default.
- W2971692007 hasConcept C2524010 @default.
- W2971692007 hasConcept C30475298 @default.
- W2971692007 hasConcept C32891209 @default.