Scali Maria Chiara, Zagatina Angela, Simova Iana, Zhuravskaya Nadezhda, Ciampi Quirino, Paterni Marco, Marzilli Mario, Carpeggiani Clara, Picano Eugenio
Cardiology Division, Nottola Hospital, Siena, Italy; Cardiothoracic Department, Cisanello, Pisa, Italy.
Cardiology Department, Medika Cardiocenter, Saint Petersburg, Russian Federation.
Ultrasound Med Biol. 2017 Nov;43(11):2558-2566. doi: 10.1016/j.ultrasmedbio.2017.07.007. Epub 2017 Sep 1.
Various lung ultrasound (LUS) scanning modalities have been proposed for the detection of B-lines, also referred to as ultrasound lung comets, which are an important indication of extravascular lung water at rest and after exercise stress echo (ESE). The aim of our study was to assess the lung water spatial distribution (comet map) at rest and after ESE. We performed LUS at rest and immediately after semi-supine ESE in 135 patients (45 women, 90 men; age 62 ± 12 y, resting left ventricular ejection fraction = 41 ± 13%) with known or suspected heart failure or coronary artery disease. B-lines were measured by scanning 28 intercostal spaces (ISs) on the antero-lateral chest, 2nd-5th IS, along with the midaxillary (MA), anterior axillary (AA), mid-clavicular (MC) and parasternal (PS) lines. Complete 28-region, 16-region (3rd and 4th IS), 8-region (3rd IS), 4-region (3rd IS, only AA and MA) and 1-region (left 3rd IS, MA) scans were analyzed. In each space, the B-lines were counted from 0 = black lung to 10 = white lung. Interpretable images were obtained in all spaces (feasibility = 100 %). B-lines (>0 in at least 1 space) were present at ESE in 93 patients (69%) and absent in 42. More B-lines were found in the 3rd IS and along AA and MA lines. The B-line cumulative distribution was symmetric at rest (right/left = 1.10) and asymmetric with left lung predominance during stress (right/left = 0.67). The correlation of per-patient B-line number between 28-S and 16-S (R = 0.9478), 8-S (R = 0.9478) and 4-S scan (R = 0.9146) was excellent, but only good with 1-S (R = 0.8101). The average imaging and online analysis time were 5 s per space. In conclusion, during ESE, the comet map of lung water accumulation follows a predictable spatial pattern with wet spots preferentially aligned with the third IS and along the AA and MA lines. The time-saving 4-region scan is especially convenient during stress, simply dismissing dry regions and focusing on wet regions alone.
为检测B线(也称为超声肺彗星征),人们提出了多种肺部超声(LUS)扫描方式,B线是静息状态及运动负荷超声心动图(ESE)后血管外肺水的重要指标。我们研究的目的是评估静息状态及ESE后肺水的空间分布(彗星图)。我们对135例已知或疑似心力衰竭或冠状动脉疾病的患者(45例女性,90例男性;年龄62±12岁,静息左心室射血分数=41±13%)进行了静息状态下及半卧位ESE后即刻的LUS检查。通过扫描前外侧胸部第2 - 5肋间、28个肋间间隙(IS),以及腋中线(MA)、腋前线(AA)、锁骨中线(MC)和胸骨旁线(PS)来测量B线。分析了完整的28区、16区(第3和4肋间)、8区(第3肋间)、4区(第3肋间,仅AA和MA)和1区(左第3肋间,MA)扫描。在每个间隙,B线从0(肺野黑色)到10(肺野白色)进行计数。所有间隙均获得了可解读图像(可行性=100%)。93例患者(69%)在ESE时有B线(至少1个间隙>0),42例无B线。在第3肋间以及沿AA和MA线发现更多B线。B线累积分布在静息时对称(右/左=1.10),应激时不对称,左肺占优势(右/左=0.67)。每位患者28区与16区(R=0.9478)、8区(R=0.9478)和4区扫描(R=0.9146)的B线数量相关性极佳,但与1区扫描(R=0.8101)仅为良好。每个间隙的平均成像和在线分析时间为5秒。总之,在ESE期间,肺水积聚的彗星图遵循可预测的空间模式,湿区优先与第3肋间以及沿AA和MA线对齐。省时的4区扫描在应激期间特别方便,只需忽略干燥区域,仅关注湿润区域即可。