| Literature DB >> 25636383 |
Michaela Huber1, Christoph Eder2, Markus Loibl3, Arne Berner4, Johannes Zellner5, Richard Kujat6, Michael Nerlich7, Sebastian Gehmert8.
Abstract
BACKGROUND: The application of radiofrequency energy (RFE) has become widespread for surgical performed chondroplasty especially due to the anticipated sealing effect, however the safety of this procedure in the wrist remains unclear. The purpose of this study was to investigate the subchondral temperature during radiofrequency energy (RFE) application simulating chondroplasty in an arthroscopic setting of the wrist.Entities:
Mesh:
Year: 2015 PMID: 25636383 PMCID: PMC4316647 DOI: 10.1186/s12891-015-0460-2
Source DB: PubMed Journal: BMC Musculoskelet Disord ISSN: 1471-2474 Impact factor: 2.362
Figure 1Temperature sensing elements (TSE) were placed adjacent to sensible structures in the wrist in order to monitor temperature changes. TSE 1 was used as a reference to detect the temperature of the irrigation fluid at room temperature of 20°C. Seven TSEs were implanted under direct visualization to: radial recess (rr), scapho-lunate ligament (sl), dorsal site and subchondral to the center of the lunate fossa (fl), intra-articularly at the distal radioulnar joint (druj), extra-articular tendon sheath of the 4/5 compartment (4/5), ulnar nerve in alignment to the extra-articular ulno-carpal joint (un), intra-articular at the center of the midcarpal joint (mc).
Figure 2Mean temperatures were recorded for all temperature sensing elements and displayed from 0 to 60 seconds for both RFE devices (A) bipolar, (B) monopolar.
Bipolar Device
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| 0 s | 20,52 ± 1,00 | 21,61 ± 1,48 | 21,35 ± 1,48 | 21,42 ± 0,93 | 21,94 ± 1,23 | 21,62 ± 0,68 | 21,04 ± 0,74 | 22,03 ± 1,05 |
| 5 s | 21,02 ± 1,34 | 23,10 ± 1,89 | 21,46 ± 1,59 | 22,93 ± 1,04 | 22,23 ± 1,43 | 21,81 ± 0,65 | 21,07 ± 0,74 | 22,76 ± 1,50 |
| 10 s | 21,02 ± 1,34 | 24,81 ± 5,25 | 21,95 ± 1,90 | 30,03 ± 12,63 | 22,55 ± 1,61 | 21,91 ± 0,69 | 21,07 ± 0,74 | 22,74 ± 1,37 |
| 15 s | 21,24 ± 1,47 | 25,03 ± 3,36 | 22,11 ± 2,54 | 33,54 ± 14,30 | 24,08 ± 4,42 | 21,98 ± 0,75 | 21,08 ± 0,73 | 22,88 ± 1,52 |
| 20 s | 21,31 ± 1,52 | 24,61 ± 2,75 | 22,90 ± 3,00 | 31,60 ± 7,16 | 24,91 ± 5,87 | 22,11 ± 0,83 | 21,08 ± 0,75 | 22,89 ± 1,48 |
| 30 s | 20,54 ± 0,96 | 24,35 ± 2,32 | 23,80 ± 3,91 | 33,42 ± 8,49 | 27,10 ± 11,55 | 22,37 ± 1,22 | 21,08 ± 0,73 | 22,88 ± 1,15 |
| 40 s | 21,03 ± 1,31 | 24,93 ± 2,97 | 24,64 ± 4,42 | 40,16 ± 11,42 | 27,72 ± 11,81 | 22,63 ± 2,13 | 21,07 ± 0,72 | 23,43 ± 1,93 |
| 45 s | 21,23 ± 1,49 | 24,93 ± 3,15 | 25,52 ± 4,30 | 38,24 ± 9,36 | 28,40 ± 10,27 | 22,71 ± 2,26 | 21,07 ± 0,74 | 23,50 ± 2,20 |
| 60 s | 21,45 ± 1,62 | 24,54 ± 2,00 | 25,61 ± 4,80 | 27,82 ± 3,55 | 26,29 ± 6,08 | 23,09 ± 3,00 | 21,10 ± 0,72 | 23,51 ± 1,70 |
Monopolar Device
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| 0 s | 20,75 ± 1,45 | 21,85 ± 0,74 | 22,19 ± 1,02 | 21,64 ± 1,00 | 22,10 ± 0,56 | 21,78 ± 0,78 | 21,39 ± 1,28 | 22,02 ± 0,54 |
| 5 s | 20,91 ± 1,53 | 22,35 ± 1,46 | 23,16 ± 1,51 | 24,07 ± 2,93 | 22,48 ± 1,07 | 22,13 ± 1,23 | 21,67 ± 1,74 | 22,92 ± 1,39 |
| 10 s | 20,91 ± 1,53 | 22,41 ± 1,47 | 23,83 ± 1,66 | 25,88 ± 5,02 | 22,86 ± 1,44 | 22,20 ± 1,24 | 21,84 ± 2,03 | 23,27 ± 1,71 |
| 15 s | 20,96 ± 1,59 | 22,56 ± 1,46 | 24,19 ± 2,05 | 26,99 ± 6,52 | 23,06 ± 1,52 | 22,24 ± 1,24 | 21,82 ± 2,04 | 23,54 ± 1,93 |
| 20 s | 20,99 ± 1,65 | 22,65 ± 1,49 | 24,52 ± 2,58 | 29,02 ± 8,08 | 23,21 ± 1,58 | 22,34 ± 1,15 | 21,85 ± 2,03 | 23,49 ± 1,68 |
| 30 s | 20,69 ± 1,34 | 23,09 ± 1,71 | 25,08 ± 3,19 | 31,66 ± 7,94 | 23,87 ± 2,26 | 22,52 ± 1,09 | 21,89 ± 2,02 | 23,65 ± 1,73 |
| 40 s | 20,87 ± 1,42 | 23,77 ± 2,34 | 24,88 ± 3,11 | 30,91 ± 5,50 | 24,30 ± 3,09 | 22,54 ± 1,27 | 21,90 ± 2,04 | 23,80 ± 1,97 |
| 45 s | 20,94 ± 1,46 | 24,15 ± 2,26 | 24,96 ± 2,96 | 29,71 ± 3,97 | 24,38 ± 3,13 | 22,62 ± 1,37 | 21,92 ± 2,04 | 23,83 ± 2,04 |
| 60 s | 20,98 ± 1,50 | 23,82 ± 2,18 | 24,23 ± 2,33 | 27,42 ± 3,91 | 24,52 ± 3,20 | 22,75 ± 1,48 | 21,99 ± 2,08 | 23,38 ± 1,53 |
Figure 3Mean temperatures were recorded from the sensing element at the subchondral lunate fossa during bipolar and monoplar RFE application. The mean temperature in the lunate fossa was significantly higher for the bipolar system when compared to the monopolar system (*** p < 0.001).
Figure 4The maximum temperature of 69.21°C was detected in the lunate fossa for the bipolar system whereas the peak temperature was only 49.35°C for the monoplar system at the same location. In addition, peak temperature in the DRUJ reached 54.15°C when using the bipolar system but only 31.81°C for the monoploar application. The temperature of 50°C was never exceeded when using the monopolar system.