National Library of Energy BETA

Sample records for 586-5640 cf-1 whitaker

  1. Low Wind Speed Technology Phase II: Investigation of the Application of Medium-Voltage Variable-Speed Drive Technology to Improve the Cost of Energy from Low Wind Speed Turbines; Behnke, Erdman and Whitaker Engineering, Inc.

    SciTech Connect (OSTI)

    Not Available

    2006-03-01

    This fact sheet describes a subcontract with Behnke, Erdman & Whitaker Engineering, Inc. to test the feasibility of applying medium-voltage variable-speed drive technology to low wind speed turbines.

  2. One West Third Street Tulsa, Oklahoma

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Beth Whitaker Administrative Officer Springfield Maintenance Special thanks to: Ron Beck ... "The individual Corps districts know what type of maintenance work needs to be done at ...

  3. Microsoft Word - Memo to the Secretary.doc

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    http://www.cfo.doe.gov/cf1-2/2007afr.pdf

  4. Climate Time-Machine

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Climate Time-Machine Climate Time-Machine 20th Century Reanalysis Project Explores Earth's Past and Future Climate January 25, 2011 Berkeley Lab Contact: Jon Bashor, jbashor@lbl.gov, +1 510 486 5849 Wiley-Blackwell Contact: Ben Norman, lifesciencenews@wiley.com,+44(0)1243 770 375 Science Contact: Jeffrey Whitaker, Jeffrey.S.Whitaker@noaa.gov, +1 303 497 6313 2011-01-25-20C-Climate.jpg A dust storm approaching Stratford, TX on April 18, 1935. The 20th Century Reanalysis Project will provide

  5. Turbocharged Spark Ignited Direct Injection - A Fuel Economy Solution for

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    The US | Department of Energy Turbocharged Spark Ignited Direct Injection - A Fuel Economy Solution for The US Turbocharged Spark Ignited Direct Injection - A Fuel Economy Solution for The US Turbocharged SIDI is the most promising advanced gasoline technology; combines existing & proven technologies in a synergistic manner, offers double digit fuel economy benefits, much lower cost than diesel or hybrid. deer09_whitaker.pdf (488.25 KB) More Documents & Publications E85 Optimized

  6. EM SSAB CHAIRS Bi-Monthly Conference Call

    Office of Environmental Management (EM)

    August 27, 2013 Participants Board Chairs/Representatives Site Staff Hanford Steve Hudson, Susan Leckband Kim Ballinger, Michael Turner Idaho Herb Bohrer Peggy Hinman Nevada Donna Hruska Kelly Snyder, Barbara Ulmer Northern New Mexico Carlos Valdez Lee Bishop, Menice Santistevan Oak Ridge David Hemelright Melyssa Noe, Spencer Gross, Pete Osborne Paducah Ralph Young Buz Smith, Eric Roberts Portsmouth Greg Simonton, Julie Galloway Savannah River Donald Bridges Gerri Flemming, Ashley Whitaker

  7. Thermal And-Or Near Infrared At Coso Geothermal Area (1968-1971...

    Open Energy Info (EERE)

    DOE-funding Unknown Exploration Basis Fumarolic and hot springs activity Notes Color IR photography References Koenig, J.B.; Gawarecki, S.J.; Austin, C.F. (1 February 1972)...

  8. Microsoft Word - Mpublic207_090607160623

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    IMPROVED TEST METHOD TO VERIFY THE POWER RATING OF A PHOTOVOLTAIC (PV) PROJECT A.Kimber 1 , T.Dierauf 1 , L.Mitchell 2 , C.Whitaker 3 , T.Townsend 3 , J.NewMiller 3 , D.King 4 , J.Granata 4 K.Emery 5 , C.Osterwald 5 , D.Myers 5 , B.Marion 5 , A.Pligavko 6 , A.Panchula 6 , T.Levitsky 6 , J.Forbess 6, F.Talmud 7 1. SunPower Corporation 2. San Francisco Public Utilities Commission 3. BEW Engineering 4. Sandia National Laboratories 5. National Renewable Energy Laboratory 6. First Solar, Inc 7.

  9. RECONCILING THE OBSERVED STAR-FORMING SEQUENCE WITH THE OBSERVED STELLAR MASS FUNCTION

    SciTech Connect (OSTI)

    Leja, Joel; Van Dokkum, Pieter G.; Franx, Marijn; Whitaker, Katherine E.

    2015-01-10

    We examine the connection between the observed star-forming sequence (SFR ? M {sup ?}) and the observed evolution of the stellar mass function in the range 0.2 < z < 2.5. We find that the star-forming sequence cannot have a slope ? ? 0.9 at all masses and redshifts because this would result in a much higher number density at 10 < log (M/M {sub ?}) < 11 by z = 1 than is observed. We show that a transition in the slope of the star-forming sequence, such that ? = 1 at log (M/M {sub ?}) < 10.5 and ? = 0.7-0.13z (Whitaker et al.) at log (M/M {sub ?}) > 10.5, greatly improves agreement with the evolution of the stellar mass function. We then derive a star-forming sequence that reproduces the evolution of the mass function by design. This star-forming sequence is also well described by a broken power law, with a shallow slope at high masses and a steep slope at low masses. At z = 2, it is offset by ?0.3 dex from the observed star-forming sequence, consistent with the mild disagreement between the cosmic star formation rate (SFR) and recent observations of the growth of the stellar mass density. It is unclear whether this problem stems from errors in stellar mass estimates, errors in SFRs, or other effects. We show that a mass-dependent slope is also seen in other self-consistent models of galaxy evolution, including semianalytical, hydrodynamical, and abundance-matching models. As part of the analysis, we demonstrate that neither mergers nor hidden low-mass quiescent galaxies are likely to reconcile the evolution of the mass function and the star-forming sequence. These results are supported by observations from Whitaker et al.

  10. United States Government Department Memorandum

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Department Memorandum DATE: September 20, 2006 Audit Report Number: OAS-L-06-20 REPLY TO ATTN OF: IG-34 (A06TG036) SUBJECT: Special Report on "The Department's Security over Personally Identifiable Information" TO: Chief Financial Officer, CF-1 Chief Human Capital Officer, HR-1 Chief Information Officer, IM-1 INTRODUCTION AND OBJECTIVE * The Department of Energy (Department) maintains'numerous information systems that contain personally identifiable information (PI). In response to

  11. Maquoketa paleotopography key to reservoirs in western Illinois

    SciTech Connect (OSTI)

    Whitaker, S.T.; Ledbetter, J.C.

    1996-08-12

    Shallow Silurian reservoirs in western Illinois have been a primary target for exploration since the late 1950s. It was not until the discovery and development of Buckhorn Consolidated field in the early 1980s, however, that significant drilling efforts for Silurian reservoirs were focused on western Illinois. At Buckhorn, 1.7 million bbl of oil have been produced from a basal Silurian dolomite at about 650 ft. Drawn by inexpensive drilling and available acreage, hundreds of operators flocked to western Illinois to try their luck. By the late 1980s, however, exploration efforts in western Illinois were curtailed due to the failure to locate additional significant reservoirs. Much of this failure was due to the lack of a suitable geologic model that could be used to explain the reason for reservoir development and thereby guide exploration efforts. An article by Whitaker and Howard in 1995 presented a geologic model explaining Silurian reservoir development and stratigraphic entrapment of oil at Buckhorn Consolidated field were formed as Silurian dolomite in-filled a shallow paleovalley cut into the underlying Ordovician Maquoketa shale. Some companies have recently initiated new exploration efforts in the area using this model. This paper discusses the efforts and results of several of these new areas.

  12. United States Goverment Department of Energy Memorandum DATE: December 11, 2007 Audit Report Number: OAS-L-08-03

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    (08-93) United States Goverment Department of Energy Memorandum DATE: December 11, 2007 Audit Report Number: OAS-L-08-03 REPLY TO ATTN OF: IG-34 (A07GT010) SUBJECT: Report on "The Department of Energy's Implementation of Revised OMB Circular No. A-123" TO: Chief Financial Officer, CF-1 INTRODUCTION AND OBJECTIVE The Office of Management and Budget's (OMB) revised Circular No. A-123 (A-123) requires Federal agencies to assess, document and test their internal controls over financial

  13. United States Government Department of Energy Memorandum OFFICE OF INSPECTOR GENERAL

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    28/07 10:24 FAX 301 903 4656 CAPITAL REGION [a 002 DOE F 1325.8 (08-93) United States Government Department of Energy Memorandum OFFICE OF INSPECTOR GENERAL DATE: November 28, 2007 REPLY TO ATTN OF: IG-34 (A07TG029) . Audit Report No.: OAS-L-08-02 SUBJECT: Report on "Department's Implementation of the Strateg:ic Integrated Procurement Enterprise System - Overall Project Planning" TO: Chief Financial Officer, CF-1 INTRODUCTION AND OBJECTIVE On September 28, 2007, we issued a report on

  14. Microsoft Word - PSRP June 5 2009 _LGPO_ OMB with minor errors fixedMBF.docm

    Broader source: Energy.gov (indexed) [DOE]

    PSRP Name: Innovative Technology Loan Guarantee Program PSRP Lead Program Office and/or Laboratory/Site Office: Loan Guarantee Program Office (LGPO) PSRP Lead Manager: Douglas Schultz Phone: 202-586-8336 E-mail: lgprogram@hq.doe.gov Address: LGPO Forrestal Bldg. CF 1.3 1000 Independence Ave, SW Washington, D.C. 20585 Does this program align with an existing PART program? N Does this program align with an existing CFDA program? N Program Title: Innovative Technology Loan Guarantee Program

  15. Monitoring the fate of radionuclides released to the environment: May 1991 report

    SciTech Connect (OSTI)

    Bauer, L.R.

    1992-08-13

    A review of the radiological effluent and environmental monitoring practices in use at Mound has been conducted. The radionuclides under consideration were HT, Pu-239, U-233,234, U-238, Th-230, Th-232, Co-60, Cs-137, and Ac-227. It is concluded from this analysis that additional continuous monitoring programs are not warranted. Dose contributions from these radionuclides are negligible. Further, in many cases environmental surveillance would not be practical due to the extremely low concentrations encountered in the offsite environment. For these reasons, it is believed that no additional action is required in response to DOE Tiger Team Finding R/CF-1.

  16. Universidad del Turabo Final Report: Juracan Energy Team

    Broader source: Energy.gov (indexed) [DOE]

    (08-93) United States Goverment Department of Energy Memorandum DATE: December 11, 2007 Audit Report Number: OAS-L-08-03 REPLY TO ATTN OF: IG-34 (A07GT010) SUBJECT: Report on "The Department of Energy's Implementation of Revised OMB Circular No. A-123" TO: Chief Financial Officer, CF-1 INTRODUCTION AND OBJECTIVE The Office of Management and Budget's (OMB) revised Circular No. A-123 (A-123) requires Federal agencies to assess, document and test their internal controls over financial

  17. Thermoelasticity of SSP Materials: An Integrated Ultrasonic and X-radiation Study

    SciTech Connect (OSTI)

    Baosheng Li

    2008-07-29

    It has been a very productive year for accomplishing the tasks outlined in the original proposal. Quite a few crystalline materials [tantalum (Ta), molybdenum (Mo), cerium (Ce) beryllium (Be)] and amorphous materials [zirconium tungstate (ZrW2O8), SiO2, and germanium diselenide (GeSe2) glasses] have been assessed at high pressures up to 12 GPa and acoustic velocities and densities have been obtained simultaneously using our unique technique. Major activities include sample preparation, high pressure cell assembly testing, and conducting ultrasonic and X-ray diffraction measurements at BNL as well as resonance ultrasonic spectroscopy (RUS) measurements at UCLA on appropriate samples. Sample preparations for Ce and Be were made at Los Alamos National Lab for which special grades and specialized machining of the sample are required. Pilot experiments for optimizing high pressure cell assemblies were conducted using the 1000-ton multi-anvil press (USCA-1000) in the High Pressure Lab at Stony Brook, and simultaneous ultrasonic and X-ray diffraction experiments were conducted using the DDIA apparatus installed at X17B2 of NSLS at BNL. New data analysis protocols have been developed for deriving density of amorphous materials at high pressure and therefore its equation of state. Following on previous years effort, attempts have been made to derive single crystal elastic constants based on the current measurements on polycrystalline samples at high pressure in conjunction with previous data as well as the current RUS measurements at ambient conditions. Single crystal elastic constants of Tantalum have been measured using RUS techniques at room pressure and high temperature. Educational and training opportunities have been provided for postdoctoral associate researchers, Drs. Wei Liu (project leader for Mo, and ZrW2O8 and SiO2 glass) and Qiong Liu (Ta project leader) and graduate students Mr. Matthew Whitaker (Project Ce and FeSi) and Sytle Antao (GeSe2 glass project). A

  18. Janus Experiments: Data from Mouse Irradiation Experiments 1972 - 1989

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    The Janus Experiments, carried out at Argonne National Laboratory from 1972 to 1989 and supported by grants from the US Department of Energy, investigated the effects of neutron and gamma radiation on mouse tissues primarily from B6CF1 mice. 49,000 mice were irradiated: Death records were recorded for 42,000 mice; gross pathologies were recorded for 39,000 mice; and paraffin embedded tissues were preserved for most mice. Mouse record details type and source of radiation [gamma, neutrons]; dose and dose rate [including life span irradiation]; type and presence/absence of radioprotector treatment; tissue/animal morphology and pathology. Protracted low dose rate treatments, short term higher dose rate treatments, variable dose rates with a same total dose, etc. in some cases in conjunction with radioprotectors, were administered. Normal tissues, tumors, metastases were preserved. Standard tissues saved were : lung, liver, spleen, kidney, heart, any with gross lesions (including mammary glands, Harderian gland with eye, adrenal gland, gut, ovaries or testes, brain and pituitary, bone). Data are searchable and specimens can be obtained by request.

  19. ARM - Midlatitude Continental Convective Clouds (jensen-sonde)

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Jensen, Mike; Comstock, Jennifer; Genio, Anthony Del; Giangrande, Scott; Kollias, Pavlos

    2012-01-19

    A major component of the Mid-latitude Continental Convective Clouds Experiment (MC3E) field campaign was the deployment of an enhanced radiosonde array designed to capture the vertical profile of atmospheric state variables (pressure, temperature, humidity wind speed and wind direction) for the purpose of deriving the large-scale forcing for use in modeling studies. The radiosonde array included six sites (enhanced Central Facility [CF-1] plus five new sites) launching radiosondes at 3-6 hour sampling intervals. The network will cover an area of approximately (300)2 km2 with five outer sounding launch sites and one central launch location. The five outer sounding launch sites are: S01 Pratt, KS [ 37.7oN, 98.75oW]; S02 Chanute, KS [37.674, 95.488]; S03 Vici, Oklahoma [36.071, -99.204]; S04 Morris, Oklahoma [35.687, -95.856]; and S05 Purcell, Oklahoma [34.985, -97.522]. Soundings from the SGP Central Facility during MC3E can be retrieved from the regular ARM archive. During routine MC3E operations 4 radiosondes were launched from each of these sites (approx. 0130, 0730, 1330 and 1930 UTC). On days that were forecast to be convective up to four additional launches were launched at each site (approx. 0430, 1030, 1630, 2230 UTC). There were a total of approximately 14 of these high frequency launch days over the course of the experiment.

  20. Radioprotectors and Tumors: Molecular Studies in Mice

    SciTech Connect (OSTI)

    Gayle Woloschak, David Grdina

    2010-03-10

    This proposal investigated effects of radiation using a set of archival tissues. Main interests of this proposal were to investigate effects of irradiation alone or in the presence or radioprotectors; to investigate these effects on different tissues; and to use/develop molecular biology techniques that would be suitable for work with archived tissues. This work resulted in several manuscripts published or in preparation. Approach for evaluation of gene copy numbers by quantitative real time PCR has been developed and we are striving to establish methods to utilize Q-RT-PCR data to evaluate genomic instability caused by irradiation(s) and accompanying treatments. References: 1. Paunesku D, Paunesku T, Wahl A, Kataoka Y, Murley J, Grdina DJ, Woloschak GE. Incidence of tissue toxicities in gamma ray and fission neutron-exposed mice treated with Amifostine. Int J Radiat Biol. 2008, 84(8):623-34. PMID: 18661379, http://informahealthcare.com/doi/full/10.1080/09553000802241762?cookieSet=1 2. Wang Q, Paunesku T and Woloschak GE. Tissue and data archives from irradiation experiments conducted at Argonne National Laboratory over a period of four decades, in press in Radiation and Environmental Biophysics. 3. Alcantara M, Paunesku D, Rademaker A, Paunesku T and Woloschak GE. A RETROSPECTIVE ANALYSIS OF TISSUE TOXICITIES IN B6CF1 MICE IRRADIATED WITH FISSION NEUTRONS OR COBALT 60 GAMMA RAYS: Gender modulates accumulation of tissue toxicities caused by low dose rate fractionated irradiation; in preparation; this document has been uploaded as STI product 4. Wang Q, Paunesku T Wanzer B and Woloschak GE. Mitochondrial gene copy number differences in different tissues of irradiated and control mice with lymphoid cancers; in preparation 5. Wang Q, Raha, S, Paunesku T and Woloschak GE. Evaluation of gene copy number differences in different tissues of irradiated and control mice; in preparation

  1. Gravitational waves and stalled satellites from massive galaxy mergers at z ? 1

    SciTech Connect (OSTI)

    McWilliams, Sean T.; Pretorius, Frans; Ostriker, Jeremiah P.

    2014-07-10

    We present a model for merger-driven evolution of the mass function for massive galaxies and their central supermassive black holes at late times. We discuss the current observational evidence in favor of merger-driven massive galaxy evolution during this epoch, and demonstrate that the observed evolution of the mass function can be reproduced by evolving an initial mass function under the assumption of negligible star formation. We calculate the stochastic gravitational wave signal from the resulting black hole binary mergers in the low redshift universe (z ? 1) implied by this model, and find that this population has a signal-to-noise ratio 2 × to 5 × larger than previous estimates for pulsar timing arrays, with a (2?, 3?) lower limit within this model of h{sub c}(f = 1 yr{sup –1}) = (1.1 × 10{sup –15}, 6.8 × 10{sup –16}). The strength of this signal is sufficient to make it detectable with high probability under conservative assumptions within the next several years. A principle reason that this result is larger than previous estimates is our use of a recent recalibration of the black hole-stellar mass correlation for the brightest cluster galaxies, which increases our estimate by a factor of ?2 relative to past results. For cases where a galaxy merger fails to lead to a black hole merger, we estimate the probability for a given number of satellite black holes to remain within a massive host galaxy, and interpret the result in light of ULX observations. We find that in rare cases, wandering supermassive black holes may be bright enough to appear as ULXs.

  2. Sister Dehalobacter Genomes Reveal Specialization in Organohalide Respiration and Recent Strain Differentiation Likely Driven by Chlorinated Substrates

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Tang, Shuiquan; Wang, Po Hsiang; Higgins, Steven A.; Löffler, Frank E.; Edwards, Elizabeth A.

    2016-02-12

    Here we report that the genomes of two closely related Dehalobacter strains (strain CF and strain DCA) were assembled from the metagenome of an anaerobic enrichment culture that reductively dechlorinates chloroform (CF), 1,1,1-trichloroethane (1,1,1-TCA) and 1,1-dichloroethane (1,1-DCA). The 3.1 Mbp genomes of strain CF (that dechlorinates CF and 1,1,1-TCA) and strain DCA (that dechlorinates 1,1-DCA) each contain 17 putative reductive dehalogenase homologous (rdh) genes. These two genomes were systematically compared to three other available organohalide-respiring Dehalobacter genomes (Dehalobacter restrictus strain PER-K23, Dehalobacter sp. strain E1 and Dehalobacter sp. strain UNSWDHB), and to the genomes of Dehalococcoides mccartyi strain 195 andmore » Desulfitobacterium hafniense strain Y51. This analysis compared 42 different metabolic and physiological categories. The genomes of strains CF and DCA share 90% overall average nucleotide identity and >99.8% identity over a 2.9 Mbp alignment that excludes large insertions, indicating that these genomes differentiated from a close common ancestor. This differentiation was likely driven by selection pressures around two orthologous reductive dehalogenase genes, cfrA and dcrA, that code for the enzymes that reduce CF or 1,1,1-TCA and 1,1-DCA. The many reductive dehalogenase genes found in the five Dehalobacter genomes cluster into two small conserved regions and were often associated with Crp/Fnr transcriptional regulators. Specialization is on-going on a strain-specific basis, as some strains but not others have lost essential genes in the Wood-Ljungdahl (strain E1) and corrinoid biosynthesis pathways (strains E1 and PER-K23). The gene encoding phosphoserine phosphatase, which catalyzes the last step of serine biosynthesis, is missing from all five Dehalobacter genomes, yet D. restrictus can grow without serine, suggesting an alternative or unrecognized biosynthesis route exists. In contrast to D. mccartyi, a

  3. ARM - Midlatitude Continental Convective Clouds - Ultra High Sensitivity Aerosol Spectrometer(tomlinson-uhsas)

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Tomlinson, Jason; Jensen, Mike

    2012-02-28

    Ultra High Sensitivity Aerosol Spectrometer (UHSASA) A major component of the Mid-latitude Continental Convective Clouds Experiment (MC3E) field campaign was the deployment of an enhanced radiosonde array designed to capture the vertical profile of atmospheric state variables (pressure, temperature, humidity wind speed and wind direction) for the purpose of deriving the large-scale forcing for use in modeling studies. The radiosonde array included six sites (enhanced Central Facility [CF-1] plus five new sites) launching radiosondes at 3-6 hour sampling intervals. The network will cover an area of approximately (300)2 km2 with five outer sounding launch sites and one central launch location. The five outer sounding launch sites are: S01 Pratt, KS [ 37.7oN, 98.75oW]; S02 Chanute, KS [37.674, 95.488]; S03 Vici, Oklahoma [36.071, -99.204]; S04 Morris, Oklahoma [35.687, -95.856]; and S05 Purcell, Oklahoma [34.985, -97.522]. Soundings from the SGP Central Facility during MC3E can be retrieved from the regular ARM archive. During routine MC3E operations 4 radiosondes were launched from each of these sites (approx. 0130, 0730, 1330 and 1930 UTC). On days that were forecast to be convective up to four additional launches were launched at each site (approx. 0430, 1030, 1630, 2230 UTC). There were a total of approximately 14 of these high frequency launch days over the course of the experiment. These files contain brightness temperatures observed at Purcell during MC3E. The measurements were made with a 5 channel (22.235, 23.035, 23.835, 26.235, 30.000GHz) microwave radiometer at one minute intervals. The results have been separated into daily files and the day of observations is indicated in the file name. All observations were zenith pointing. Included in the files are the time variables base_time and time_offset. These follow the ARM time conventions. Base_time is the number seconds since January 1, 1970 at 00:00:00 for the first data point of the file and time_offset is

  4. ARM - Midlatitude Continental Convective Clouds Microwave Radiometer Profiler (jensen-mwr)

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Jensen, Mike

    2012-02-01

    A major component of the Mid-latitude Continental Convective Clouds Experiment (MC3E) field campaign was the deployment of an enhanced radiosonde array designed to capture the vertical profile of atmospheric state variables (pressure, temperature, humidity wind speed and wind direction) for the purpose of deriving the large-scale forcing for use in modeling studies. The radiosonde array included six sites (enhanced Central Facility [CF-1] plus five new sites) launching radiosondes at 3-6 hour sampling intervals. The network will cover an area of approximately (300)2 km2 with five outer sounding launch sites and one central launch location. The five outer sounding launch sites are: S01 Pratt, KS [ 37.7oN, 98.75oW]; S02 Chanute, KS [37.674, 95.488]; S03 Vici, Oklahoma [36.071, -99.204]; S04 Morris, Oklahoma [35.687, -95.856]; and S05 Purcell, Oklahoma [34.985, -97.522]. Soundings from the SGP Central Facility during MC3E can be retrieved from the regular ARM archive. During routine MC3E operations 4 radiosondes were launched from each of these sites (approx. 0130, 0730, 1330 and 1930 UTC). On days that were forecast to be convective up to four additional launches were launched at each site (approx. 0430, 1030, 1630, 2230 UTC). There were a total of approximately 14 of these high frequency launch days over the course of the experiment. These files contain brightness temperatures observed at Purcell during MC3E. The measurements were made with a 5 channel (22.235, 23.035, 23.835, 26.235, 30.000GHz) microwave radiometer at one minute intervals. The results have been separated into daily files and the day of observations is indicated in the file name. All observations were zenith pointing. Included in the files are the time variables base_time and time_offset. These follow the ARM time conventions. Base_time is the number seconds since January 1, 1970 at 00:00:00 for the first data point of the file and time_offset is the offset in seconds from base_time.