icf
Differences
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| Both sides previous revisionPrevious revisionNext revision | Previous revision | ||
| icf [2026/07/28 18:48] – andrew | icf [2026/08/12 10:40] (current) – reno | ||
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| |Dead time (sec)| Dead time the instrument is set to| | |Dead time (sec)| Dead time the instrument is set to| | ||
| |WL cal step number| Current cal step for the instrument | | |WL cal step number| Current cal step for the instrument | | ||
| - | |Unused| | | + | |Slitmask Motor Delay|Multi-board electronics - This is the slitmask delay between moving from one slit to the next. The typical value for this is 80\\ New Electronics - This sets the speed of the slitmask motor, typically and usually left at 14.| |
| |Umkehr Offset| Azimuth offset during Umkehr measurements | | |Umkehr Offset| Azimuth offset during Umkehr measurements | | ||
| |ND filter 0| Filer correction from Neutral Density (ND) filter #0 | | |ND filter 0| Filer correction from Neutral Density (ND) filter #0 | | ||
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| |Zenith steps/rev| The number of steps to perform a complete rotation of the zenith | | |Zenith steps/rev| The number of steps to perform a complete rotation of the zenith | | ||
| |Brewer Type| Version of Brewer spectrophotometer | | |Brewer Type| Version of Brewer spectrophotometer | | ||
| - | |COM Port #| | | + | |COM Port #| Select the comport being used. **if using dosbox or similar dos emulator, this is not the actual comport used on the computer, but the comport specified in the config. Typically left as 1| |
| |o3 Temp coef hg| | | |o3 Temp coef hg| | | ||
| |n2 Temp coef hg| | | |n2 Temp coef hg| | | ||
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| |NO2/O3 Mode Change| | | |NO2/O3 Mode Change| | | ||
| |Grating Slope| The relationship of movement between micrometer #1 and micrometer #2 to maximize counts| | |Grating Slope| The relationship of movement between micrometer #1 and micrometer #2 to maximize counts| | ||
| - | |Grating Intercept| | | + | |Grating Intercept|:::| |
| |Micrometer Zero| | | |Micrometer Zero| | | ||
| |Iris Open Steps| The number of steps it takes to open the Iris | | |Iris Open Steps| The number of steps it takes to open the Iris | | ||
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| |NO2 FW#1 Pos| Position of filter wheel #1 during a Nitrogen dioxide measurement| | |NO2 FW#1 Pos| Position of filter wheel #1 during a Nitrogen dioxide measurement| | ||
| | O3 FW#1 Pos| Position of filter wheel #1 during Ozone measurements | | | O3 FW#1 Pos| Position of filter wheel #1 during Ozone measurements | | ||
| - | | FW#2 Pos| Position of filter wheel #2 during any SL measurement/ | + | | SL FW#2 Pos| Position of filter wheel #2 during any tests or measurements that use the standard lamp | |
| | uv FW#2 Pos| Position of filter wheel #2 during a UV measurment | | | uv FW#2 Pos| Position of filter wheel #2 during a UV measurment | | ||
| |Zenith Offset| Offset from the zenith zero positioning for optimal pointing | | |Zenith Offset| Offset from the zenith zero positioning for optimal pointing | | ||
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| |Release date| Date that the ICF was created| | |Release date| Date that the ICF was created| | ||
| |EXTRAS| | | |EXTRAS| | | ||
| - | |AUTO HG| | | + | |AUTO HG|Allows the software to automatically insert HG as required when running a schedule with auto routine. Typically an HG is ran every 2 hours or a change in temperature of 2 degrees, which ever happens first. \\ 0 - Disable \\ 1 - Enable| |
| - | |FW2 oscil| | | + | |FW2 oscil|Allows filterwheel 2 to keep changing with no limits during DS measurements. This usually happens when the sun gets covered/ |
| |HG FW#2 Pos| Position of filter wheel #2 when using the Hg bulb | | |HG FW#2 Pos| Position of filter wheel #2 when using the Hg bulb | | ||
| |Low Signal limit| The number of counts at which the instrument will switch to a lower neutral density filter or skip the test during a direct sun measurement| | |Low Signal limit| The number of counts at which the instrument will switch to a lower neutral density filter or skip the test during a direct sun measurement| | ||
| |Upper Signal limit| The number of counts at which the instrument will increase the neutral density filter during a direct sun measurement| | |Upper Signal limit| The number of counts at which the instrument will increase the neutral density filter during a direct sun measurement| | ||
| - | |Use cubic DSP| | | + | |Use cubic DSP|Enable the use of cubic dispersion. \\ 0 - Disable \\ 1 - Enable| |
| |Skip DS if too dim| Enable skipping a Direct Sun (DS) measurement if counts are too low | | |Skip DS if too dim| Enable skipping a Direct Sun (DS) measurement if counts are too low | | ||
| |O3ETC-R6| Ozone Extraterrestrial Constant (ETC) minus the R6 standard lamp ratio | | |O3ETC-R6| Ozone Extraterrestrial Constant (ETC) minus the R6 standard lamp ratio | | ||
| |So2ETC-R5| Sulfur dioxide Extraterrestrial Constant (ETC) minus the R5 standard lamp ratio | | |So2ETC-R5| Sulfur dioxide Extraterrestrial Constant (ETC) minus the R5 standard lamp ratio | | ||
| - | |PHYCS alpha / slits 2-5 / o3 | | | + | |PHYCS alpha / slits 2-5 / o3 | PHYCS correction factor for stray light on slits 2 - 5 | |
| - | |PHYCS beta / slit 1 / so2 | | | + | |PHYCS beta / slit 1 / so2 | PHYCS correction factor for stray light on slit 1 | |
| - | |Apply PHYCS| | | + | |Apply PHYCS| |
| |Updated with CF| | | |Updated with CF| | | ||
icf.1785264515.txt.gz · Last modified: 2026/07/28 18:48 by andrew