Parameter |
Description |
Units |
Comment |
air_temp |
Air temperature |
degrees C |
Taken ~2 m above the ground, averaged over 1 min |
humidity |
Relative humidity |
% |
Taken ~2 m above the ground, averaged over 1 min. Sensors have non-linearity around 30%, values larger than 100% (see Known Issues) |
wind_speed |
Wind speed |
km/h |
Taken ~2 m above the ground, averaged over 1 min. Mechanical sensors sometimes get stuck (see Known Issues) |
wind_direction |
Wind direction |
degrees east of north |
Taken ~2 m above the ground, averaged over 1 min. Mechanical sensors sometimes get stuck, some offsets exist (see Known Issues) |
pressure |
Barometric air pressure |
mbar (=hPa) |
Taken ~2 m above the ground, averaged over 1 min |
solar_rad |
Solar irradiation |
W/m^2 |
Averaged over 1 min |
soil_temp |
Soil temperature |
degrees C |
Taken ~10 cm below the surface, averaged over 1 min |
net_rad |
Net radiation |
W/m^2 |
Difference between the downward and upward energy fluxes, measured ~2 m above the ground, averaged over 1 min |
heat_flux |
Ground heat flux |
W/m^2 |
Heat flux measured ~10 cm below the surface, averaged over 1 min. Flux sensors installed upside down at some sites (see Known Issues) |
Parameter |
Description |
Units |
Comment |
seeing_6pt |
Seeing (6-pt extrap.) |
arcsec |
Seeing corrected to zenith for a wavelength of 500 nm and extrapolated to 0 ms from 6 different exposure times [~6, 12, 18, 24, 30, 36 ms] using an exponential function.
This is the preferred seeing measurement of the TMT DIMMs. |
seeing_2pt |
Seeing (2-pt extrap.) |
arcsec |
Seeing corrected to zenith for a wavelength of 500 nm and extrapolated to 0 ms from
2 different exposure times [~6, 12 ms] using the extrapolation of
Tokovinin (2002). |
strehl[12] |
Strehl ratio |
none |
Average Strehl ratios of the two star images on the DIMM CCD. Note that due to a bug in the code, the
value of the Strehl ratios in the database is off by a multiplicative factor (see Known Issues). |
airmass |
Air mass |
none |
Air mass of the DIMM observation |
star |
Star ID |
none |
Star ID in form 'XXX XXX', for example, 'Alp Eri'. This is the same for DIMM and MASS. |
exposure |
Exposure time |
ms |
Exposure time of the individual DIMM images. The value for this parameter is 5 ms for all data in the database. This is, however, simply the exposure time as set
in the configuration files. The real exposure time is ~6 ms. |
points_good |
Number good data points |
none |
Number of valid one-dimensional (1d) DIMM exposures used for a seeing measurement. Exposures are checked
for star flux, star image positions etc. before being used in the seeing calculation. |
points_all |
Number all data points |
none |
Number of all 1d DIMM exposures taken for a seeing measurement. The value for this parameter is 6000 for all data in the database. |
fluxes[12] |
Measured star flux |
Counts |
Integrated fluxes of the two stellar images averaged over all valid 1d DIMM frames |
fluxesb |
Measured background flux |
Counts/pixel |
Mean background level averaged over all valid 1d DIMM frames |
peak_flux[12] |
Peak flux |
CCD counts |
Flux in the brightest pixels in the two stellar images, averaged over all valid 1d DIMM images |
scintillation[12] |
Scintillation index |
none |
Scintillation index of the integrated flux in the valid 1d images |
star_pos_[12] |
Average star position |
pixel |
Average position of the stellar image centroids in the 1d DIMM images |
star_pos_sep |
Average star separation |
pixel |
Average separation of the two star images |
star_pos_s[12][if] |
Initial/final star position |
pixel |
Initial and final positions of the two star images on the CCD. This is used to assess tracking performance of the telescope. |
Parameter |
Description |
Units |
Comment |
fixed_cn2_[123456] |
Layer strength |
m^1/3 |
Strengths of the MASS layers (note that this is Cn2*dh, not Cn2) when using a 6-layer profile with fixed layer altitudes. |
fixed_seecn |
Seeing from Cn2 profile |
arcsec |
Free atmosphere seeing calculated from the fixed_cn2 values. This is the most reliable seeing measurement from the MASS. |
fsee |
Free atmosphere seeing from turbulence moments |
arcsec |
Free atmosphere seeing calculated directly from the turbulence moments. This works even if the Cn2 profile restoration fails
(or its error estimate is deemed too high), but it is usually a less reliable value than
fixed_seecn. |
isopl |
Isoplanatic angle from turbulence moments |
arcsec |
Isoplanatic angle calculated from turbulence moments. It is recommended that this value is not used, but that the
isoplanatic angle is calculated directly from the
fixed_cn2 values as this results in a more reliable estimate. |
tau |
Coherence time from turbulence moments |
ms |
Turbulence coherence time calculated from turbulence moments. This is the best estimate of tau0 available from the MASS, but it
requires some postprocessing. If you are not familiar with this, we strongly recommend that you read some of the publications
on the topic. |
fixed_z_[123456] |
Layer altitude |
km |
Altitudes of the MASS layers when using a 6-layer profile with fixed layer altitudes. For our data, these values are always
0.5, 1, 2, 4, 8 and 16 km. |
float_cn2_[123] |
Floating model layer strength |
m^1/3 |
Strengths of the MASS layers (note that this is Cn2*dh, not Cn2) when using a 3-layer profile with variable layer altitudes. |
float_z_[123] |
Floating model layer altitude |
km |
Altitudes of the MASS layers when using a 3-layer profile with variable layer altitudes. |
Other MASS parameters |
|
|
For descriptions of other parameters, please download the Turbina User Guide from the Documentation page of the
MASS Group. If you need any of those parameters for your
analysis, you are probably aware of this anyway (or you should be). |