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(Standard Edition)
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Views to Expect
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Exact filter bandpass will vary based on final telescope application, so no specific FWHM bandpass is designated. Now observers can buy a filter based on their desired observing goals instead of their budget. Choose Prominence Model for more and WIDER prominences with a little surface. |
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Exact filter bandpass will vary based on final telescope application, so no specific FWHM bandpass is designated. Now observers can buy a filter based on their desired observing goals instead of their budget. Choose Chromosphere MORE surface contrast and narrower prominences. |
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Filters with 0.8 Ångstrom bandwidths will reveal prominences in high contrast.
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Filters with 0.7 Ångstrom bandwidths will reveal prominences in high contrast and occasionally, surface texture. Prominences are generally larger with 0.7Å filters than in narrower bandwidths.
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Filters with 0.6 Ångstrom bandwidths will reveal some surface contrast as well as prominences. 0.6Å filter can be a good compromise for those having a difficult decision.
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Filters with 0.5 Ångstrom bandwidths will reveal better surface contrast as well as great prominences.
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Filters with 0.4 Ångstrom bandwidths will reveal excellent surface contrast as well as fine chromosphere detail. Filaments are clearly depicted with a 0.4Å FWHM filter.
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Filters with 0.3 Ångstrom bandwidths will reveal superior surface contrast above any other filter. Views are generally somewhat dimmer. Expect "Pencil-Thin" details on surface and prominence features.
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