User manual VAISALA SKY CONDITION ALGORITHM BROCHURE FOR VAISALA CEILOMETER CL31
DON'T FORGET : ALWAYS READ THE USER GUIDE BEFORE BUYING !!!
If this document matches the user guide, instructions manual or user manual, feature sets, schematics you are looking for, download it now. Diplodocs provides you a fast and easy access to the user manual VAISALA SKY CONDITION ALGORITHM. We hope that this VAISALA SKY CONDITION ALGORITHM user guide will be useful to you.
You may also download the following manuals related to this product:
VAISALA SKY CONDITION ALGORITHM BROCHURE (264 ko)
Manual abstract: user guide VAISALA SKY CONDITION ALGORITHMBROCHURE FOR VAISALA CEILOMETER CL31
Detailed instructions for use are in the User's Guide.
[. . . ] Box 26, FIN-00421 Helsinki, FINLAND Tel: +358 9 894 91 Fax: +358 9 8949 2485 Email: metsales@vaisala. com www. vaisala. com
Sky Condition Algorithm for Vaisala Ceilometer CL31
Features/Benefits
· Produces sky condition information from a single ceilometer · New calculation algorithm - good results compared to human observers · Optional for the CL31 ceilometer · Generally used in automatic surface weather stations and airport weather monitoring systems
The CL31 ceilometer can be configured to report sky condition automatically and accurately.
The Vaisala Sky Condition algorithm is an easy and cost-effective way to produce more information from ceilometer data. [. . . ] The new algorithm computes in 2D time-height domain.
Reliable results with automatic measurement
The new Sky Condition Algorithm has shown good results in comparison to sky condition reported by human observers (1. For comparison, success percentage values for the ASOS ceilometer algorithm (2, CT25K embedded algorithm and the new Sky Condition algorithm are presented in table 1.
Picture of whole sky from one point
The purpose of the algorithm is to construct an image of the whole sky based on the ceilometer measurements only from one single point. The sky condition algorithm uses a time series of ceilometer data to calculate the cloud amount of different cloud layers and the corresponding layer heights. Sky Condition algorithms are generally used in automatic surface weather stations and in airport weather monitoring systems.
SKY CONDITION ALGORITHM FOR CL31
CLOUD HEIGHT
Technical Data
Data collection
A new sky condition message is calculated every five (5) minutes based on data collected during the last 30 minutes. The last 10 minutes are double-weighted.
Compatibility
Vaisala Sky Condition algorithm is fully supported by CL-View Graphical User Interface for Ceilometers. Sky Condition message can be viewed either in the main window or in a separate window. CL-View provides cloud layer height and information in either text or symbol format.
Data display
The Sky Condition message line is included in the CL31 Ceilometer data message 2 and its subclass. The message output interval is the same as the ceilometer data acquisition interval.
Message line
The Sky Condition message line in data message 2 and its subclass is: 1 055 3 170 6 230 0 /// 0 /// where: 1 the first number of the line: detection status as follows: 0 . . . [. . . ] American Meteorological Society.
(2
Specifications subject to change without prior notice. [. . . ]
DISCLAIMER TO DOWNLOAD THE USER GUIDE VAISALA SKY CONDITION ALGORITHM
Click on "Download the user Manual" at the end of this Contract if you accept its terms, the downloading of the manual VAISALA SKY CONDITION ALGORITHM will begin.