DQR ID | Subject | Data Streams Affected |
---|---|---|
D010423.16 | SGP/SIRS/E16 - Diffuse Pyranometer Thermal Offsets | sgpsirsE16.a0, sgpsirsE16.a1 |
D010423.17 | SGP/SIRS/E18 - Diffuse Pyranometer Thermal Offsets | sgpsirsE18.a0, sgpsirsE18.a1 |
D010423.18 | SGP/SIRS/E19 - Diffuse Pyranometer Thermal Offsets | sgpsirsE19.a0, sgpsirsE19.a1 |
D010423.19 | SGP/SIRS/E20 - Diffuse Pyranometer Thermal Offsets | sgpsirsE20.a0, sgpsirsE20.a1 |
D010423.21 | SGP/SIRS/E22 - Diffuse Pyranometer Thermal Offsets | sgpsirsE22.a0, sgpsirsE22.a1 |
D040525.10 | SGP/SIRS/E19 - Metadata errors | sgpsirsE19.a0, sgpsirsE19.a1 |
D990716.20 | SGP/SIRS - SIRS E16 April 1999 (SERI-QC Results) | sgpsirsE16.a0, sgpsirsE16.a1 |
D990716.21 | SGP/SIRS - SIRS E18 April 1999 (SERI-QC Results) | sgpsirsE18.a0, sgpsirsE18.a1 |
D990716.23 | SGP/SIRS - SIRS E19 April 1999 (Part 2 of 7) | sgpsirsE19.a0, sgpsirsE19.a1 |
D990716.25 | SGP/SIRS - SIRS E19 April 1999 (Part 4 of 7) | sgpsirsE19.a0, sgpsirsE19.a1 |
D990716.27 | SGP/SIRS - SIRS E19 April 1999 (Part 6 of 7) | sgpsirsE19.a0, sgpsirsE19.a1 |
D990716.29 | SGP/SIRS - SIRS E20 April 1999 | sgpsirsE20.a0, sgpsirsE20.a1 |
D990716.30 | SGP/SIRS - SIRS E22 April 1999 | sgpsirsE22.a0, sgpsirsE22.a1 |
Start Date | Start Time | End Date | End Time |
---|---|---|---|
08/21/1997 | 0735 | 02/21/2001 | 1620 |
Subject: | SGP/SIRS/E16 - Diffuse Pyranometer Thermal Offsets |
DataStreams: | sgpsirsE16.a0, sgpsirsE16.a1 |
Description: | Broadband downwelling shortwave diffuse (sky) irradiance measurements available from SIRS during the period of this Data Quality Report (DQR), require adjustment for thermal offsets. These thermal, or ?zero? offsets refer to the generally reduced output signals from a shaded pyranometer due to the exchange of longwave (infrared) irradiance between the single black thermopile detector, the protective glass domes surrounding the detector, and the atmosphere. Originally considered an acceptable nighttime response of thermopile-type pyranometers, the generally negative bias is now recognized to significantly effect the accuracy of SIRS diffuse irradiance data during daylight periods. Studies of the Eppley Laboratory, Inc. Model PSP (Precision Spectral Pyranometer), used for the SIRS measurements of diffuse irradiance, suggest the thermal offset correction can range from near 0 to as much as 30 Watts per square meter, depending on the coincident net longwave, or infrared irradiance [1, 2]. Under very clear-sky conditions, the diffuse irradiance from a shaded PSP can be less than the minimum physical limit defined by radiative transfer model estimates based only on Rayleigh scattering effects. A correction method has been developed for adjusting SIRS diffuse irradiance data [3]. The resulting Value Added Product (VAP) will be applied to SIRS data for the period of this DQR. The VAP will not be applied to SIROS data collected before the instrument platform was converted to SIRS. Additionally, the Model PSP radiometer has been replaced by a Model 8-48 which uses a black and white thermopile detector known to reduce the thermal offset errors to less than 2 Watts per square meter [3]. The radiometer replacement at this SIRS location was completed on the ending date of this DQR. References: 1. Gulbrandsen, A., 1978: On the use of pyranometers in the study of spectral solar radiation and atmospheric aerosols. J. Appl. Meteorol., 17, 899-904. 2. Cess, R. D., X. Jing, T. Qian, and M. Sun, 1999: Validation strategies applied to the measurement of total, direct and diffuse shortwave radiation at the surface. J. Geophys. Res. 3. Dutton, E.G., J. Michalsky, T. Stoffel, B. Forgan, J. Hickey, D. Nelson, T. Alberta, and I. Reda, 2001: Measurement of Broadband Diffuse Solar Irradiance Using Current Commercial Instrumentation With a Correction for Thermal Offset Errors. J. Atmos. Oceanic Tech. Vol 18, No. 3, 297-314. (March 2001) |
Measurements: | sgpsirsE16.a0:
sgpsirsE16.a1:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
10/15/1997 | 0825 | 02/20/2001 | 2220 |
Subject: | SGP/SIRS/E18 - Diffuse Pyranometer Thermal Offsets |
DataStreams: | sgpsirsE18.a0, sgpsirsE18.a1 |
Description: | Broadband downwelling shortwave diffuse (sky) irradiance measurements available from SIRS during the period of this Data Quality Report (DQR), require adjustment for thermal offsets. These thermal, or ?zero? offsets refer to the generally reduced output signals from a shaded pyranometer due to the exchange of longwave (infrared) irradiance between the single black thermopile detector, the protective glass domes surrounding the detector, and the atmosphere. Originally considered an acceptable nighttime response of thermopile-type pyranometers, the generally negative bias is now recognized to significantly effect the accuracy of SIRS diffuse irradiance data during daylight periods. Studies of the Eppley Laboratory, Inc. Model PSP (Precision Spectral Pyranometer), used for the SIRS measurements of diffuse irradiance, suggest the thermal offset correction can range from near 0 to as much as 30 Watts per square meter, depending on the coincident net longwave, or infrared irradiance [1, 2]. Under very clear-sky conditions, the diffuse irradiance from a shaded PSP can be less than the minimum physical limit defined by radiative transfer model estimates based only on Rayleigh scattering effects. A correction method has been developed for adjusting SIRS diffuse irradiance data [3]. The resulting Value Added Product (VAP) will be applied to SIRS data for the period of this DQR. The VAP will not be applied to SIROS data collected before the instrument platform was converted to SIRS. Additionally, the Model PSP radiometer has been replaced by a Model 8-48 which uses a black and white thermopile detector known to reduce the thermal offset errors to less than 2 Watts per square meter [3]. The radiometer replacement at this SIRS location was completed on the ending date of this DQR. References: 1. Gulbrandsen, A., 1978: On the use of pyranometers in the study of spectral solar radiation and atmospheric aerosols. J. Appl. Meteorol., 17, 899-904. 2. Cess, R. D., X. Jing, T. Qian, and M. Sun, 1999: Validation strategies applied to the measurement of total, direct and diffuse shortwave radiation at the surface. J. Geophys. Res. 3. Dutton, E.G., J. Michalsky, T. Stoffel, B. Forgan, J. Hickey, D. Nelson, T. Alberta, and I. Reda, 2001: Measurement of Broadband Diffuse Solar Irradiance Using Current Commercial Instrumentation With a Correction for Thermal Offset Errors. J. Atmos. Oceanic Tech. Vol 18, No. 3, 297-314. (March 2001) |
Measurements: | sgpsirsE18.a0:
sgpsirsE18.a1:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
07/08/1998 | 0145 | 02/22/2001 | 1535 |
Subject: | SGP/SIRS/E19 - Diffuse Pyranometer Thermal Offsets |
DataStreams: | sgpsirsE19.a0, sgpsirsE19.a1 |
Description: | Broadband downwelling shortwave diffuse (sky) irradiance measurements available from SIRS during the period of this Data Quality Report (DQR), require adjustment for thermal offsets. These thermal, or ?zero? offsets refer to the generally reduced output signals from a shaded pyranometer due to the exchange of longwave (infrared) irradiance between the single black thermopile detector, the protective glass domes surrounding the detector, and the atmosphere. Originally considered an acceptable nighttime response of thermopile-type pyranometers, the generally negative bias is now recognized to significantly effect the accuracy of SIRS diffuse irradiance data during daylight periods. Studies of the Eppley Laboratory, Inc. Model PSP (Precision Spectral Pyranometer), used for the SIRS measurements of diffuse irradiance, suggest the thermal offset correction can range from near 0 to as much as 30 Watts per square meter, depending on the coincident net longwave, or infrared irradiance [1, 2]. Under very clear-sky conditions, the diffuse irradiance from a shaded PSP can be less than the minimum physical limit defined by radiative transfer model estimates based only on Rayleigh scattering effects. A correction method has been developed for adjusting SIRS diffuse irradiance data [3]. The resulting Value Added Product (VAP) will be applied to SIRS data for the period of this DQR. The VAP will not be applied to SIROS data collected before the instrument platform was converted to SIRS. Additionally, the Model PSP radiometer has been replaced by a Model 8-48 which uses a black and white thermopile detector known to reduce the thermal offset errors to less than 2 Watts per square meter [3]. The radiometer replacement at this SIRS location was completed on the ending date of this DQR. References: 1. Gulbrandsen, A., 1978: On the use of pyranometers in the study of spectral solar radiation and atmospheric aerosols. J. Appl. Meteorol., 17, 899-904. 2. Cess, R. D., X. Jing, T. Qian, and M. Sun, 1999: Validation strategies applied to the measurement of total, direct and diffuse shortwave radiation at the surface. J. Geophys. Res. 3. Dutton, E.G., J. Michalsky, T. Stoffel, B. Forgan, J. Hickey, D. Nelson, T. Alberta, and I. Reda, 2001: Measurement of Broadband Diffuse Solar Irradiance Using Current Commercial Instrumentation With a Correction for Thermal Offset Errors. J. Atmos. Oceanic Tech. Vol 18, No. 3, 297-314. (March 2001) |
Measurements: | sgpsirsE19.a1:
sgpsirsE19.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
02/13/1998 | 0532 | 02/20/2001 | 1850 |
Subject: | SGP/SIRS/E20 - Diffuse Pyranometer Thermal Offsets |
DataStreams: | sgpsirsE20.a0, sgpsirsE20.a1 |
Description: | Broadband downwelling shortwave diffuse (sky) irradiance measurements available from SIRS during the period of this Data Quality Report (DQR), require adjustment for thermal offsets. These thermal, or ?zero? offsets refer to the generally reduced output signals from a shaded pyranometer due to the exchange of longwave (infrared) irradiance between the single black thermopile detector, the protective glass domes surrounding the detector, and the atmosphere. Originally considered an acceptable nighttime response of thermopile-type pyranometers, the generally negative bias is now recognized to significantly effect the accuracy of SIRS diffuse irradiance data during daylight periods. Studies of the Eppley Laboratory, Inc. Model PSP (Precision Spectral Pyranometer), used for the SIRS measurements of diffuse irradiance, suggest the thermal offset correction can range from near 0 to as much as 30 Watts per square meter, depending on the coincident net longwave, or infrared irradiance [1, 2]. Under very clear-sky conditions, the diffuse irradiance from a shaded PSP can be less than the minimum physical limit defined by radiative transfer model estimates based only on Rayleigh scattering effects. A correction method has been developed for adjusting SIRS diffuse irradiance data [3]. The resulting Value Added Product (VAP) will be applied to SIRS data for the period of this DQR. The VAP will not be applied to SIROS data collected before the instrument platform was converted to SIRS. Additionally, the Model PSP radiometer has been replaced by a Model 8-48 which uses a black and white thermopile detector known to reduce the thermal offset errors to less than 2 Watts per square meter [3]. The radiometer replacement at this SIRS location was completed on the ending date of this DQR. References: 1. Gulbrandsen, A., 1978: On the use of pyranometers in the study of spectral solar radiation and atmospheric aerosols. J. Appl. Meteorol., 17, 899-904. 2. Cess, R. D., X. Jing, T. Qian, and M. Sun, 1999: Validation strategies applied to the measurement of total, direct and diffuse shortwave radiation at the surface. J. Geophys. Res. 3. Dutton, E.G., J. Michalsky, T. Stoffel, B. Forgan, J. Hickey, D. Nelson, T. Alberta, and I. Reda, 2001: Measurement of Broadband Diffuse Solar Irradiance Using Current Commercial Instrumentation With a Correction for Thermal Offset Errors. J. Atmos. Oceanic Tech. Vol 18, No. 3, 297-314. (March 2001) |
Measurements: | sgpsirsE20.a1:
sgpsirsE20.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
11/25/1997 | 0630 | 02/21/2001 | 2000 |
Subject: | SGP/SIRS/E22 - Diffuse Pyranometer Thermal Offsets |
DataStreams: | sgpsirsE22.a0, sgpsirsE22.a1 |
Description: | Broadband downwelling shortwave diffuse (sky) irradiance measurements available from SIRS during the period of this Data Quality Report (DQR), require adjustment for thermal offsets. These thermal, or ?zero? offsets refer to the generally reduced output signals from a shaded pyranometer due to the exchange of longwave (infrared) irradiance between the single black thermopile detector, the protective glass domes surrounding the detector, and the atmosphere. Originally considered an acceptable nighttime response of thermopile-type pyranometers, the generally negative bias is now recognized to significantly effect the accuracy of SIRS diffuse irradiance data during daylight periods. Studies of the Eppley Laboratory, Inc. Model PSP (Precision Spectral Pyranometer), used for the SIRS measurements of diffuse irradiance, suggest the thermal offset correction can range from near 0 to as much as 30 Watts per square meter, depending on the coincident net longwave, or infrared irradiance [1, 2]. Under very clear-sky conditions, the diffuse irradiance from a shaded PSP can be less than the minimum physical limit defined by radiative transfer model estimates based only on Rayleigh scattering effects. A correction method has been developed for adjusting SIRS diffuse irradiance data [3]. The resulting Value Added Product (VAP) will be applied to SIRS data for the period of this DQR. The VAP will not be applied to SIROS data collected before the instrument platform was converted to SIRS. Additionally, the Model PSP radiometer has been replaced by a Model 8-48 which uses a black and white thermopile detector known to reduce the thermal offset errors to less than 2 Watts per square meter [3]. The radiometer replacement at this SIRS location was completed on the ending date of this DQR. References: 1. Gulbrandsen, A., 1978: On the use of pyranometers in the study of spectral solar radiation and atmospheric aerosols. J. Appl. Meteorol., 17, 899-904. 2. Cess, R. D., X. Jing, T. Qian, and M. Sun, 1999: Validation strategies applied to the measurement of total, direct and diffuse shortwave radiation at the surface. J. Geophys. Res. 3. Dutton, E.G., J. Michalsky, T. Stoffel, B. Forgan, J. Hickey, D. Nelson, T. Alberta, and I. Reda, 2001: Measurement of Broadband Diffuse Solar Irradiance Using Current Commercial Instrumentation With a Correction for Thermal Offset Errors. J. Atmos. Oceanic Tech. Vol 18, No. 3, 297-314. (March 2001) |
Measurements: | sgpsirsE22.a0:
sgpsirsE22.a1:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
07/08/1998 | 0145 | 03/31/2001 | 2359 |
Subject: | SGP/SIRS/E19 - Metadata errors |
DataStreams: | sgpsirsE19.a0, sgpsirsE19.a1 |
Description: | The latitude, longitude and altitude of the El Reno (E19) site were incorrectly entered into the ARM database. The correct location of the SIRS.E19 instrument is: Lat: 35.557N Lon: 98.017W Alt: 421m |
Measurements: | sgpsirsE19.a1:
sgpsirsE19.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/01/1999 | 0001 | 04/30/1999 | 2359 |
Subject: | SGP/SIRS - SIRS E16 April 1999 (SERI-QC Results) |
DataStreams: | sgpsirsE16.a0, sgpsirsE16.a1 |
Description: | Data quality for this site is very good this month. Just under 100% - of the daytime data are present. Passing or low-level flags are assigned to 95.4% of the present daytime data. On the mornings of the 5th and 6th low-level flags indicate that the DS is too low or the DD or NIP too high by the three-component test. The DS and DD were forced below daytime empirical limits by heavily overcast skies on the afternoon of the 13th, and again on the 24th. The NIP also went below empirical limits for a few minutes shortly after noon on the 13th.The DD filed is filled with "-99999" missing data for 43 minutes on the morning of the 21st. At 537 GMT on the 18th the UIR increases to nearly twice normal nighttime levels and becomes quite noisy. The signal does not recover by the end of the month. No problems were observed in the DIR or US signals. |
Measurements: | sgpsirsE16.a0:
sgpsirsE16.a1:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/01/1999 | 0001 | 04/30/1999 | 2359 |
Subject: | SGP/SIRS - SIRS E18 April 1999 (SERI-QC Results) |
DataStreams: | sgpsirsE18.a0, sgpsirsE18.a1 |
Description: | Data quality at this site is good this month. All of the daytime data are present. Passing or low-level flags are assigned to 90.6% of the present daytime data. Data labeled strange-but-true make up another 6.5% of the present daytime data. Low to moderate flags observed in the early morning hours indicate that the DS is too low by the three-component test, or that the NIP or DD is too high. Heavily overcast skies cause the DD and DS to fall below daytime empirical limits on a number of occasions. Just before noon on the 3rd, and again for a few minutes late in the afternoon on the 24th, the DS falls below daytime empirical limits, but the DD and NIP are (moderately) flagged too high by the two-component test (Gompertz boundaries.) Around noon on the 5th and 6th the DS is too low by the three-component test, but for a short time close to noon on the 5th the DS falls into the physically impossible region where Kn > Kt. No problems noted in the DIR, UIR or US signals. |
Measurements: | sgpsirsE18.a0:
sgpsirsE18.a1:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/03/1999 | 0001 | 04/04/1999 | 2130 |
Subject: | SGP/SIRS - SIRS E19 April 1999 (Part 2 of 7) |
DataStreams: | sgpsirsE19.a0, sgpsirsE19.a1 |
Description: | Missing data due to data ingest failure. |
Measurements: | sgpsirsE19.a1:
sgpsirsE19.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/07/1999 | 1901 | 04/09/1999 | 2000 |
Subject: | SGP/SIRS - SIRS E19 April 1999 (Part 4 of 7) |
DataStreams: | sgpsirsE19.a0, sgpsirsE19.a1 |
Description: | Missing due to data ingest problems. |
Measurements: | sgpsirsE19.a1:
sgpsirsE19.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/22/1999 | 1801 | 04/24/1999 | 2000 |
Subject: | SGP/SIRS - SIRS E19 April 1999 (Part 6 of 7) |
DataStreams: | sgpsirsE19.a0, sgpsirsE19.a1 |
Description: | Missing data due to problems with ingest. |
Measurements: | sgpsirsE19.a1:
sgpsirsE19.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/01/1999 | 0001 | 04/30/1999 | 2359 |
Subject: | SGP/SIRS - SIRS E20 April 1999 |
DataStreams: | sgpsirsE20.a0, sgpsirsE20.a1 |
Description: | Good data quality for this site this month. All data are present, and 92.5% of the present daytime data earn passing or low-level flags. Another 6.1% of the daytime data are flagged strange-but-true. Low-level flags in the early morning hours shortly after sunrise indicate that the DS is too low, or the NIP or DD too high by the three-component test. Low-level flags seen after noon in the second half of the month indicate that the DS is too high. The DS and DD are forced below daytime empirical limits by overcast skies on several occasions. Moderate to serious flags shortly after noon on the 14th indicate that the DS signal is too high by the three-component test. On the 22nd at 1605 GMT the 10m tower was taken down for upgrade. The UIR and US signal fields will be filled with the data logger missing data flag, -99999, until the new tower is installed. Otherwise, data collection will continue as usual. No problems noted in DIR signal. |
Measurements: | sgpsirsE20.a1:
sgpsirsE20.a0:
|
Start Date | Start Time | End Date | End Time |
---|---|---|---|
04/01/1999 | 0001 | 04/30/1999 | 2359 |
Subject: | SGP/SIRS - SIRS E22 April 1999 |
DataStreams: | sgpsirsE22.a0, sgpsirsE22.a1 |
Description: | Data quality is excellent at this site this month. Present daytime data is at 100%. Just over 98% of the present daytime data earn passing or low-level flags. In the first week of the month low-level flags indicate that the DS is too high by the three-component test, or that the DD or NIP is too low. Heavy cloud cover on several occasions caused the DS and DD to fall below daytime empirical limits. On the afternoon of the 14th the NIP fell below daytime empirical limits for a short time. Shortly before noon on the 26th the DS signal was above daytime empirical limits. No problems note in the DIR, UIR or US signals. |
Measurements: | sgpsirsE22.a0:
sgpsirsE22.a1:
|