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2600 Series RF Power Sensors
250 kHz to 3500 MHz High Power Transfer Standard
Advanced Energy's 2600 Series RF power standards enable the precise measurement of RF power (2.5 W to 250 W) in the 250 kHz to 3500 MHz frequency range. These standards, which are highly accurate and stable with time and temperature are ideal for the transfer of calibration factors to other high power RF standards and sensors.
特徴
• 2.5 W to 250 W dynamic range (+34 to +54 dBm)
• Highly accurate and stable with time and temperature.
メリット
• TEGAM High Power RF Calibration System Compatible
仕様
| Basic Accuracy: | 1.0% (typical |
|---|---|
| Communication: | See Power Meter specs |
| Frequency Range: | 250 kHz to 3.5 GHz |
| Power Range: | 2.5 W to 250 W |
| Power Range (typical): | 2.5 W to 250 W |
| Power Requirements: | Thermistor Power Meter Required |
技術文書
サービス
Repair
Our worldwide service centers provide fast cycle times, use only AE-qualified parts, and follow the original product's specifications and test procedures for the highest quality repair or calibration.
| Product Family | Calibration | Calibration with Alignment |
Total Support Package (TSP) |
||||||
|---|---|---|---|---|---|---|---|---|---|
| Term of Agreement | Annual | One Year | Two Years | Three Years | Five Years | One Year | Two Years | Three Years | Five Years |
| TEGAM 5540 | | | | | | | | | |
| Lumasense | | | | | | | | ||
| Plasma Power | | | | | | | |||
Calibration and Alignment
Advanced Energy has the tools and processes to ensure your equipment continues to meet its original specifications. Our products are calibrated at global AE service sites with proprietary technology designed to exceed industry standards.
| Product Family | Calibration | Calibration with Alignment |
Total Support Package (TSP) |
||||||
|---|---|---|---|---|---|---|---|---|---|
| Term of Agreement | Annual | One Year | Two Years | Three Years | Five Years | One Year | Two Years | Three Years | Five Years |
| TEGAM 5540 | | | | | | | | | |
| Lumasense | | | | | | | | ||
| Plasma Power | | | | | | | |||
